World Library  
Flag as Inappropriate
Email this Article

Leo Minor

Article Id: WHEBN0000211826
Reproduction Date:

Title: Leo Minor  
Author: World Heritage Encyclopedia
Language: English
Subject: Cancer (constellation), 46 Leonis Minoris, Jordanus (constellation), Leo (constellation), Ursa Major
Collection: Constellations, Leo Minor, Northern Constellations
Publisher: World Heritage Encyclopedia
Publication
Date:
 

Leo Minor

Leo Minor
Constellation
Leo Minor
Abbreviation LMi
Genitive Leonis Minoris
Pronunciation ,
genitive
Symbolism the lesser Lion
Right ascension 9h 22.4m to 11h 06.5m
Declination 22.84° to 41.43°[1]
Family Ursa Major
Quadrant NQ2
Area 232 sq. deg. (64th)
Main stars 3
Bayer/Flamsteed
stars
34
Stars with planets 3
Stars brighter than 3.00m 0
Stars within 10.00 pc (32.62 ly) 0
Brightest star 46 LMi (Praecipua) (3.83m)
Nearest star 11 LMi
(36.46 ly, 11.18 pc)
Messier objects 0
Meteor showers Leonis Minorids
Bordering
constellations
Ursa Major
Lynx
Cancer (corner)
Leo
Visible at latitudes between +90° and −45°.
Best visible at 21:00 (9 p.m.) during the month of April.

Leo Minor is a small and faint constellation in the northern celestial hemisphere. Its name is Latin for "the smaller lion", in contrast to Leo, the larger lion. It lies between the larger and more recognizable Ursa Major to the north and Leo to the south. Leo Minor was not regarded as a separate constellation by classical astronomers; it was designated by Johannes Hevelius in 1687.[2]

There are 37 stars brighter than apparent magnitude 6.5 in the constellation; three are brighter than magnitude 4.5. 46 Leonis Minoris, an orange giant of magnitude 3.8, is located some 95 light-years from Earth. At magnitude 4.4, Beta Leonis Minoris is the second brightest star and the only one in the constellation with a Bayer designation. It is a binary star, the brighter component of which is an orange giant and the fainter a yellow-white main sequence star. The third brightest star is 21 Leonis Minoris, a rapidly rotating white main-sequence star of average magnitude 4.5. The constellation also includes two stars with planetary systems, two pairs of interacting galaxies, and the unique deep-sky object Hanny's Voorwerp.

Contents

  • History 1
  • Characteristics 2
  • Notable features 3
    • Stars 3.1
    • Deep-sky objects 3.2
    • Meteor shower 3.3
  • See also 4
  • References 5
  • External links 6

History

The classical astronomers Aratus and Ptolemy had noted the region of what is now Leo Minor to be undefined and not containing any distinctive pattern; Ptolemy classified the stars in this area as amorphōtoi (not belonging to a constellation outline) within the constellation Leo.[3]

Johannes Hevelius first depicted Leo Minor in 1687 when he outlined ten new constellations in his star atlas Firmamentum Sobiescianum,[4] and included 18 of its objects in the accompanying Catalogus Stellarum Fixarum.[5] Hevelius decided upon Leo Minor or Leo Junior as a depiction that would align with its beastly neighbours the Lion and the Great Bear.[6] In 1845, English astronomer Francis Baily revised the catalogue of Hevelius's new constellations, and assigned a Greek letter known as Bayer designation to stars brighter than apparent magnitude 4.5.[7] Richard A. Proctor gave the constellation the name Leaena "the Lioness" in 1870,[3] explaining that he sought to shorten the constellation names to make them more manageable on celestial charts.[8]

German astronomer Velletri.[9][10] Arabist Friedrich Wilhelm Lach describes a different view, noting that they had been seen as Al Haud "the Pond", which the Gazelle jumps into.[3] In Chinese astronomy, the stars Beta, 30, 37 and 46 Leonis Minoris made up Neiping, a "Court of Judge or Mediator", or Shi "Court Eunuch"[4] or were combined with stars of the neighbouring Leo to make up a large celestial dragon or State Chariot.[3][11] A line of four stars was known as Shaowei; it represented four Imperial advisors and may have been located in Leo Minor, Leo or adjacent regions.[4]

Characteristics

A dark area of the sky with a triangle of brighter stars just visible to the naked eye in good conditions,[12] Leo Minor has been described by Patrick Moore as having "dubious claims to a separate identity".[13] It is a small constellation bordered by Ursa Major to the north, Lynx to the west, Leo to the south, and touching the corner of Cancer to the southwest. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is 'LMi'.[14] The official constellation boundaries, as set by Eugène Delporte in 1930, are defined by a polygon of 16 sides. In the equatorial coordinate system, the right ascension coordinates of these borders lie between 9h 22.4m and 11h 06.5m, while the declination coordinates are between 22.84° and 41.43°.[1] Ranked 64th out of 88 constellations in size, Leo Minor covers an area of 232.0 square degrees, or 0.562 percent of the sky.[4] It culminates each year at midnight on February 24,[12] and at 9 p.m. on May 24.[15]

Notable features

Stars

There are only three stars in the constellation brighter than magnitude 4.5,[6] and 37 stars with a magnitude brighter than 6.5.[4] Leo Minor does not have a star designated Alpha because Baily erred and allocated a Greek letter to only one star, Beta.[2] It is unclear whether he intended to give 46 Leonis Minoris a Bayer designation, as he recognised Beta and 46 Leonis Minoris as of the appropriate brightness in his catalogue. He died before revising his proofs, which might explain this star's omission.[6]

At magnitude 3.8, the brightest star in Leo Minor is an orange giant of spectral class K0III named 46 Leonis Minoris or Praecipua;[16] its colour is evident when seen through binoculars.[13] Situated 95 light-years (29 parsecs) from Earth,[2] it has around 32 times the luminosity and is 8.5 times the size of the Sun.[17] It was also catalogued and named as o Leonis Minoris by Johann Elert Bode, which has been misinterpreted as Omicron Leonis Minoris.[6] More confusion occurred with its proper name Praecipua, which appears to have been originally applied to 37 Leonis Minoris in the 1814 Palermo Catalogue of Giuseppe Piazzi, who mistakenly assessed the latter star as the brighter. This name was later connected by Allen with 46 Leonis Minoris—an error perpetuated by subsequent astronomers.[4] The original "Praecipua", 37 Leonis Minoris, has an apparent magnitude of 4.69,[18] but is a distant yellow supergiant of spectral type G2.5IIa and absolute magnitude of −1.84,[19] around 578 light-years (177 parsecs) distant.[18]

Leo Minor as seen by the naked eye

Beta Leonis Minoris is a binary star system. The primary is a giant star of spectral class G8 and apparent magnitude of 4.4. It has around double the mass, 7.8 times the radius and is 36 times the luminosity of the Earth's Sun. Separated by 11 seconds of arc from the primary, the secondary is a yellow-white main sequence star of spectral type F8. The two orbit around a common centre of gravity every 38.62 years,[17] and lie 154 light-years (47 parsecs) away from the Solar System.[20]

Around 98 light-years (30 parsecs) away and around 10 times as luminous as the Sun, 21 Leonis Minoris is a rapidly rotating white main-sequence star, spinning on its axis in less than 12 hours and very likely flattened in shape.[17] Of average apparent magnitude 4.5 and spectral type A7V, it is a Delta Scuti variable.[21] These are short period (six hours at most) pulsating stars which have been used as standard candles and as subjects to study asteroseismology.[22]

Leo Minor above the head of Leo, as depicted in Urania's Mirror, a set of constellation cards published in London c. 1825[23]

Also known as SU and SV Leonis Minoris, 10 and 11 Leonis Minoris are yellow giants of spectral type G8III, with average magnitudes 4.54 and 5.34 respectively. Both are RS Canum Venaticorum variables,[24][25] with 10 Leonis Minoris varying by 0.012 magnitude over 40.4 days, and 11 Leonis Minoris by 0.033 magnitude over 18 days.[26] 11 Leonis Minoris has a red dwarf companion of spectral type M5V and apparent magnitude 13.0.[27] 20 Leonis Minoris is a multiple star system 49 light-years (15 parsecs) away from the Sun. The main star is another yellow star, this time a dwarf of spectral type G3Va and apparent magnitude 5.4.[28] The companion is an old, active red dwarf that has a relatively high metallicity and is of spectral type M6.5. The fact that the secondary star is brighter than expected indicates it is likely two stars very close together that are unable to be made out separately with current viewing technology.[29]

R and S Leonis Minoris are long-period Mira variables, while U Leonis Minoris is a semiregular variable;[30] all three are red giants of spectral types M6.5e-M9.0e,[31] M5e [32] and M6 respectively.[33] R varies between magnitudes 6.3 and 13.2 during a period of 372 days, S varies between magnitudes 8.6 and 13.9 during a period of 234 days, and U varies between magnitudes 10.0 and 13.3 during a period of 272 days. The lack of bright stars makes finding these objects challenging for amateur astronomers.[30] G 117-B15A, also known as RY Leonis Minoris, is a pulsating white dwarf of apparent magnitude 15.5.[34] With a period of approximately 215 seconds, and losing a second every 8.9 million years, the 400-million-year-old star has been proposed as the most stable celestial clock.[35]

SX Leonis Minoris is a dwarf nova of the SU Ursae Majoris type that was identified in 1994.[36] It consists of a white dwarf and a donor star, which orbit each other every 97 minutes. The white dwarf sucks matter from the other star onto an accretion disc and heats up to between 6000 and 10000 K. The dwarf star erupts every 34 to 64 days, reaching magnitude 13.4 in these outbursts and remaining at magnitude 16.8 when quiet.[37] Leo Minor contains another dwarf nova, RZ Leonis Minoris, which brightens to magnitude 14.2 from a baseline magnitude of around 17 but does so at shorter intervals than other dwarf novae.[38]

Two stars with planetary systems have been found. HD 87883 is an orange dwarf of magnitude 7.57 and spectral type K0V 18 parsecs distant from Earth. With a diameter three quarters that of Earth's sun, it is only 31 percent as luminous. It is orbited by a planet around 1.78 times the mass of Jupiter every 7.9 years, and there are possibly other smaller planets.[39] HD 82886 is a yellow dwarf of spectral type G0 and visual magnitude 7.63.[40] A planet 1.3 times the mass of Jupiter and orbiting every 705 days was discovered in 2011.[41]

Deep-sky objects

Spiral galaxy NGC 3021 which lies about 100 million light-years away.[42]

In terms of deep-sky objects, Leo Minor contains many galaxies viewable in amateur telescopes.[43] Located 3 degrees southeast of 38 Leonis Minoris, NGC 3432 is seen nearly edge on. Known as the knitting needle galaxy, it is of apparent magnitude 11.7 and measures 6.8 by 1.4 arcminutes.[12] Located 42 million light years away, it is moving away from the Solar System at a rate of 616 km per second. In 2000, a star within the galaxy brightened to magnitude 17.4, and has since been determined to be a luminous blue variable and supernova impostor.[44] NGC 3003, a SBbc barred spiral galaxy with an apparent magnitude of 12.3 and an angular size of 5.8 arcminutes, is seen almost edge-on.[45] NGC 3344, 25 million light years distant, is face-on towards Earth.[46] Measuring 7.1 by 6.5 arcminutes in size, it has an apparent magnitude of 10.45.[47] NGC 3504 is a starburst barred spiral galaxy of apparent magnitude 11.67 and measuring 2.1 by 2.7 arcminutes.[48] It has hosted supernovae in 1998[49] and 2001.[50] It and the spiral galaxy NGC 3486 are also almost face-on towards Earth; the latter is of magnitude 11.05 and measures 7.1 by 5.2 arcminutes.[51] NGC 2859 is an SB0-type lenticular galaxy.[52]

At least two pairs of interacting galaxies have been observed. Arp 107 is a pair of galaxies in the process of merging, located 450 million light years away.[53] NGC 3395 and NGC 3396 are a spiral and irregular barred spiral galaxy respectively that are interacting, located 1.33 degrees southwest of 46 Leonis Minoris.[54]

The unique deep-sky object known as Hanny's Voorwerp was discovered in Leo Minor in 2007 by Dutch school teacher Hanny van Arkel while participating as a volunteer in the Galaxy Zoo project. Lying near the 650 million light year-distant spiral galaxy IC 2497, it is around the same size as the Milky Way.[55] It contains a 16,000 light year wide hole.[56] The voorwerp is thought to be the visual light echo of a quasar now gone inactive,[57] possibly as recently as 200,000 years ago.[55]

Meteor shower

Discovered by Dick McCloskey and Annette Posen of the Harvard Meteor Program in 1959,[58] the Leonis Minorid meteor shower peaks between October 18 and October 29. The shower's parent body is the long period comet C/1739 K1 (Zanotti).[59] It is a minor shower, and can only be seen from the Northern Hemisphere.[60]

See also

References

Citations
  1. ^ a b , Leo MinorThe ConstellationsIAU, .
  2. ^ a b c Ridpath & Tirion 2001, pp. 168–69.
  3. ^ a b c d Allen 1963, p. 263.
  4. ^ a b c d e f Filling the remaining gapsStar TalesRidpath, .
  5. ^ Hevelius 1687, pp. 214–15.
  6. ^ a b c d Wagman 2003, pp. 189–90.
  7. ^ Wagman 2003, p. 8.
  8. ^ Proctor 1870, pp. 16–17.
  9. ^ Allen 1963, p. 42.
  10. ^ See also Mark R. Chartrand III (1983) Skyguide: A Field Guide for Amateur Astronomers, p. 158 (ISBN 0-307-13667-1).
  11. ^ See also Chartrand, at p. 158.
  12. ^ a b c Thompson & Thompson 2007, p. 290.
  13. ^ a b Moore 2000, p. 103.
  14. ^ Russell 1922, p. 469.
  15. ^ The Constellations : Part 2 Culmination Times.
  16. ^ SIMBAD 46 Leonis Minoris.
  17. ^ a b c PraecipuaKaler, .
  18. ^ a b SIMBAD 37 Leonis Minoris.
  19. ^ Kovtyukh et al. 2010.
  20. ^ SIMBAD Beta Leonis Minoris.
  21. ^ SIMBAD 21 Leonis Minoris.
  22. ^ Delta Scuti and the Delta Scuti variables.
  23. ^ Ridpath, Urania’s Mirror.
  24. ^ SIMBAD 10 Leonis Minoris.
  25. ^ SIMBAD 11 Leonis Minoris.
  26. ^ Skiff & Lockwood 1986.
  27. ^ SIMBAD GJ 356 B.
  28. ^ SIMBAD 20 Leonis Minoris.
  29. ^ Gizis et al. 2000.
  30. ^ a b Levy 2005, pp. 186–87.
  31. ^ SIMBAD R Leonis Minoris.
  32. ^ SIMBAD S Leonis Minoris.
  33. ^ SIMBAD U Leonis Minoris.
  34. ^ SIMBAD RY Leonis Minoris.
  35. ^ McDonald Observatory.
  36. ^ Nogami et al. 1997.
  37. ^ Wagner et al. 1998.
  38. ^ Robertson et al. 1995.
  39. ^ Fischer et al. 2009.
  40. ^ SIMBAD HD 82886.
  41. ^ Planet HD 82886 b.
  42. ^ "A cosmological measuring tape". Retrieved 16 June 2015. 
  43. ^ Knoxville Observers – Leo Minor.
  44. ^ O'Meara 2011, p. 196.
  45. ^ NED NGC 3003.
  46. ^ galaxy in a spin.
  47. ^ NED NGC 3344.
  48. ^ NED NGC 3504.
  49. ^ Garnavich 1998.
  50. ^ Matheson et al. 2001.
  51. ^ NED NGC 3486.
  52. ^ NED NGC 2859.
  53. ^ Spitzer Arp 107.
  54. ^ Motz & Nathanson 1991, p. 180.
  55. ^ a b Hubble Zooms in on a Space Oddity.
  56. ^ Radio observations shed new light on Hanny's Voorwerp.
  57. ^ Rincon 2008.
  58. ^ Jenniskens 2006, pp. 83–84.
  59. ^ Jenniskens 2012.
  60. ^ IMO Meteor Shower Calendar 2012.

Sources

  •  
  • Fischer, Debra; Driscoll, Peter; Isaacson, Howard; Giguere, Matt; Marcy, Geoffrey W.; Valenti, Jeff; Wright, Jason T.; Henry, Gregory W.; Johnson, John Asher; Howard, Andrew; Peek, Katherine; McCarthy, Chris (2009). "Five Planets and an Independent Confirmation of HD 196885 Ab from Lick Observatory". The Astrophysical Journal 703 (2): 1545–56.  
  • Garnavich, P. (1998). "Supernova 1998cf in NGC 3504". IAU Circular 6914 (6914): 1.  
  • Gizis, J. E.; Monet, D. G.; Reid, I. N.; Kirkpatrick, J. D.; Burgasser, A. J. (2000). "Two Nearby M Dwarf Binaries from 2MASS" (abstract page).  
  • Hevelius, Johannes (1687). Catalogus Stellarum Fixarum (in Latin). Gdaņsk, Poland: Gedani, typis J.-Z. Stollii. 
  • Jenniskens, Peter (2006). Meteor Showers and their Parent Comets. Cambridge, United Kingdom: Cambridge University Press.  
  • Jenniskens, Peter (September 2012). "Mapping Meteoroid Orbits: New Meteor Showers Discovered". Sky & Telescope: 22. 
  • Kovtyukh, V. V.; Chekhonadskikh, F. A.; Luck, R. E.; Soubiran, C.; Yasinskaya, M. P.; Belik, S. I. (2010). "Accurate Luminosities for F-G Supergiants from Fe II/Fe I Line Depth Ratios". Monthly Notices of the Royal Astronomical Society 408 (3): 1568–75.  
  • Levy, David H. (2005). David Levy's Guide to Variable Stars. Cambridge, United Kingdom: Cambridge University Press.  
  • Matheson, P.; Jha, S.; Challis, P.; Kirshner, R.; Calkins, M. (2001). "Supernova 2001ac in NGC 3504". IAU Circular 7597 (7597): 3.  
  • Moore, Patrick (2000). Exploring the Night Sky with Binoculars. Cambridge, United Kingdom: Cambridge University Press.  
  • Motz, Lloyd; Nathanson, Carol (1991). The Constellations: An Enthusiast's Guide to the Night Sky. London, United Kingdom: Aurum Press.  
  • Nogami, Daisaku; Masuda, Seiji; Kato, Taichi (1997). "The 1994 Superoutburst of the New SU UMa-type Dwarf Nova, SX Leonis Minoris". Publications of the Astronomical Society of the Pacific 109: 1114–21.  
  • O'Meara, Stephen James (2011). Deep-Sky Companions: The Secret Deep. Cambridge, United Kingdom: Cambridge University Press.  
  •  
  • Ridpath, Ian; Tirion, Wil (2001). Stars and Planets Guide. Princeton University Press.  
  • Robertson, J. W.; Honeycutt, R. K.; Turner, G. W.; Honeycutt; Turner (1995). "RZ Leonis Minoris, PG 0943+521, and V1159 Orionis: Three Cataclysmic Variables with Similar and Unusual Outburst Behavior". Publications of the Astronomical Society of the Pacific 107: 443–49.  
  • Russell, Henry Norris (October 1922). "The New International Symbols for the Constellations".  
  • Skiff, Brian A.; Lockwood, G.W. (1986). "The Photometric Variability of Solar-type Stars. V. The Standard Stars 10 and 11 Leonis Minoris". Publications of the Astronomical Society of the Pacific 98 (601): 338–41.  
  • Thompson, Robert Bruce; Thompson, Barbara Fritchman (2007). Illustrated Guide to Astronomical Wonders: From Novice to Master Observer. North Sebastopol, California: O'Reilly Media.  
  • Wagman, Morton (2003). Lost Stars: Lost, Missing and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. Blacksburg, Virginia: The McDonald & Woodward Publishing Company.  
  • Wagner, R. Mark; Thorstensen, John R.; Honeycutt, R. K.; Howell, S. B.; Kaitchuck, R. H.; Kreidl, T. J.; Robertson, J. W.; Sion, E. M.; Starrfield, S. G.; Thorstensen; Honeycutt; Howell; Kaitchuck; Kreidl; Robertson; Sion; Starrfield (1998). "A Photometric and Spectroscopic Study of the Cataclysmic Variable SX Leonis Minoris in Quiescence and Superoutburst". The Astronomical Journal 109 (2): 787–800.  

Online sources

  • Baldwin, Emily (25 June 2010). "Radio observations shed new light on Hanny's Voorwerp". Astronomy Now. Pole Star Publications Ltd. Retrieved 8 November 2012. 
  • Beck, Sara J. (16 July 2010). "Delta Scuti and the Delta Scuti variables". Variable Star of the Season. AAVSO (American Association of Variable Star Observers). Retrieved 8 November 2012. 
  • "Leo Minor, Constellation Boundary". The Constellations. International Astronomical Union. Retrieved 15 October 2012. 
  • Schneider, Jean. "Planet HD 82886 b". The Extrasolar Planets Encyclopaedia. Paris Observatory. Retrieved 25 October 2012. 
  • "ESA/Hubble Picture of the Week: Galaxy in a spin". Hubble website. Retrieved 23 October 2012. 
  • "IMO Meteor Shower Calendar 2012 | International Meteor Organization". The International Meteor Organization. 1997–2012. Retrieved 31 October 2012. 
  • James, Andrew (7 February 2011). "'The '"Constellations : Part 2 Culmination Times"'". Southern Astronomical Delights. Sydney, New South Wales. Retrieved 19 October 2012. 
  • "Hubble Zooms in on a Space Oddity".  
  • Kaler, Jim. "Beta Leonis Minoris". Stars. University of Illinois. Retrieved 30 March 2007. 
  • Kaler, Jim. "21 Leonis Minoris". Stars. University of Illinois. Retrieved 15 October 2012. 
  • Kaler, Jim. "Praecipua". Stars. University of Illinois. Retrieved 15 October 2012. 
  • Grant, Shawn. "Leo Minor". Deepsky Online. Knoxville Observers. Retrieved 14 November 2012. 
  • McDonald Observatory (5 December 2005). "Astronomers Find Most Stable Optical Clock in Heavens; Aids Understanding of Stars' Lives". Phys.Org. Retrieved 22 October 2012. 
  • Jet Propulsion Laboratory, California Institute of Technology. "Results for NGC 2859". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration. Retrieved 23 October 2012. 
  • Jet Propulsion Laboratory, California Institute of Technology. "Results for NGC 3003". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration. Retrieved 23 October 2012. 
  • Jet Propulsion Laboratory, California Institute of Technology. "Results for NGC 3344". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration. Retrieved 23 October 2012. 
  • Jet Propulsion Laboratory, California Institute of Technology. "Results for NGC 3486". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration. Retrieved 23 October 2012. 
  • Jet Propulsion Laboratory, California Institute of Technology. "Results for NGC 3504". NASA/IPAC Extragalactic Database. National Aeronautics and Space Administration. Retrieved 23 October 2012. 
  •  
  •  
  •  
  •  
  • Rincon, Paul (5 August 2008). "Teacher finds new cosmic object". BBC News. Retrieved 19 October 2012. 
  • "Beta Leonis Minoris". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 8 November 2012. 
  • "SU Leonis Minoris – Variable Star of RS CVn type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 20 October 2012. 
  • "SV Leonis Minoris – Variable Star of RS CVn type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 20 October 2012. 
  • "21 Leonis Minoris – Variable Star of delta Sct type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 15 October 2012. 
  • "37 Leonis Minoris". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 5 November 2012. 
  • "46 Leonis Minoris – Variable Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 2 November 2012. 
  • "GJ 356 B – Star in double system". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 20 October 2012. 
  • "HD 82886". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 19 October 2012. 
  • "LHS 2216 – High Proper Motion Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 21 October 2012. 
  • "R Leonis Minoris – Variable Star of Mira Ceti type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 22 October 2012. 
  • "RY Leonis Minoris – Pulsating White Dwarf". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 22 October 2012. 
  • "S Leonis Minoris – Variable Star of Mira Ceti type". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 22 October 2012. 
  • "U Leonis Minoris – Semi-regular pulsating Star". SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. Retrieved 22 October 2012. 
  • "Interacting Galaxy Pair Arp 107". Spitzer Space Telescope website. Spitzer Science Center, California Institute of Technology. 9 June 2005. Retrieved 19 October 2012. 

External links

  • The Deep Photographic Guide to the Constellations: Leo Minor
  • Leo Minor at Constellation Guide

This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and USA.gov, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for USA.gov and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
 
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
 
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.
 


Copyright © World Library Foundation. All rights reserved. eBooks from Project Gutenberg are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.