Leo A Explained

Leo A
Type:IBm[1]
Dist Ly:2.6 ± 0.1 Mly (790 ± 40 kpc)[2] [3]
Z:0.000067
Appmag V:12.9
Size V:5.1 × 3.1
Constellation Name:Leo
Names:Leo III, UGC 5364, DDO 69, PGC 28868

Leo A (also known as Leo III) is an irregular galaxy that is part of the Local Group. It lies 2.6 million light-years from Earth, and was discovered by Fritz Zwicky in 1942.[4] The estimated mass of this galaxy is solar masses, with at least 80% consisting of dark matter.[5] It is one of the most isolated galaxies in the Local Group and shows no indications of an interaction or merger for several billion years. However, Leo A is nearly unique among irregular galaxies in that more than 90% of its stars formed more recently than 8 billion years ago, suggesting a rather unusual evolutionary history.[6] The presence of RR Lyrae variables shows that the galaxy has an old stellar population that is up to 10 billion years in age.[7]

The neutral hydrogen in this galaxy occupies in a volume similar to its optical extent, and is distributed in a squashed, uneven ring. The galaxy is not rotating and the hydrogen is moving about in random clumps. The proportion of elements with higher atomic numbers than helium is only about 1-2% of the ratio in the Sun. This indicates a much less complete conversion of gas into stars than in the Milky Way galaxy. The Leo A galaxy shows sign of increased star formation some time within the last 1-4 billion years, although the current level is low. There are four H II regions powered by short-lived, O-class stars.[8]

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for Leo A . 2006-11-19 .
  2. I. D. Karachentsev . V. E. Karachentseva . W. K. Hutchmeier . D. I. Makarov . A Catalog of Neighboring Galaxies . Astronomical Journal . 2004 . 12745345 . 4 . 2031–2068 . 2004AJ....127.2031K . 10.1086/382905. free .
  3. Karachentsev, I. D. . Kashibadze, O. G. . Masses of the local group and of the M81 group estimated from distortions in the local velocity field . Astrophysics . 2006 . 49 . 1 . 3–18 . 2006Ap.....49....3K . 10.1007/s10511-006-0002-6 . 120973010 .
  4. Zwicky . F . April 1942 . On the Large Scale Distribution of Matter in the Universe . Physical Review . 61 . 7–8 . 489–503 . 10.1103/PhysRev.61.489 . 1942PhRv...61..489Z .
  5. Brown, Warren R. . etal . Stellar Velocity Dispersion of the Leo A Dwarf Galaxy . September 2007 . The Astrophysical Journal . 666 . 1 . 231–235 . 10.1086/519547 . 2007ApJ...666..231B. 0705.1093 . 16639879 .
  6. Cole, Andrew . March 2007 . etal. Leo A: A Late-blooming Survivor of the Epoch of Reionization in the Local Group. The Astrophysical Journal Letters. 659. 1. L17-20. 10.1086/516711. 2007ApJ...659L..17C. astro-ph/0702646 . 14268757 .
  7. Vansevičius, Vladas . August 2008 . etal . The Full-fledged Dwarf Irregular Galaxy Leo A . The Astrophysical Journal . 611 . 2 . L93–L96 . 10.1086/423802 . 2004ApJ...611L..93V. astro-ph/0405313 . 14883376 .
  8. Young, L. M. . Lo, K. Y. . The Neutral Interstellar Medium in Nearby Dwarf Galaxies. I. Leo A . Astrophysical Journal . 462 . 203–214 . 10.1086/177141 . 1996. 1996ApJ...462..203Y.