LH 95
| LH 95 | |
|---|---|
 | |
| Observation data (J200LHA 120-N 550 epoch) | |
| Right ascension | 05h 37m 04.32s[1] |
| Declination | −66° 22′ 00.7″ |
| Distance | ~163000 light years (~50000 parsecs (50 kpc)) |
| Apparent magnitude (V) | 11.10[1] |
| Apparent dimensions (V) | 0.80' x 0.65'[1] |
| Physical characteristics | |
| Other designations | LH 95, KMHK 1139, 2MASS J05370431-6622007[1] |
| Associations | |
| Constellation | Dorado |
LH 95 is a modestly sized stellar nursery in the Large Magellanic Cloud. It is related to the HII-region LHA 120-N 55, that is, a region of hydrogen ionized by the bright stars of LH 95.
Previously only young bright stars were known in this stellar association.[2] Imaging using the Hubble Space Telescope, however, allowed the identification of more than 2,500 pre–main sequence stars with masses down to about 0.3 solar masses, thereby giving a detailed picture of what a typical stellar association in the LMC looks like.[3]
The large sample of low-mass pre–main sequence stars, stars that are currently under formation, in LH 95 allows the construction of the first most complete Initial Mass Function of an extragalactic star forming cluster.[4] The Initial Mass Function of LH 95 does not seem to differ from that typical for the Milky Way.
See also
[edit | edit source]References
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- ^ Da Rio, Nicola; Gouliermis, Dimitrios A.; Henning, Thomas, "The Complete Initial Mass Function Down to the Subsolar Regime in the Large Magellanic Cloud with Hubble Space Telescope ACS Observations", The Astrophysical Journal, Volume 696, Issue 1, pp. 528-545 (2009) ArXiv preprint
External links
[edit | edit source]- Large and small stars in harmonious coexistence
- The Hubble Heritage Project: LH 95
- NASA Astronomy Picture of the Day: Star Forming Region LH 95 (12 March 2008)
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