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Djorgovski 1 
Summary
Djorgovski 1 is a globular cluster discovered in 1986 by George Djorgovski who was looking for possible obscured globular clusters using the IRAS Point Source Catalog.[3] Studies show that its stars are "metal-poor" – they contain hydrogen and helium but little else. Djorgovski 1 is actually one of the most metal-poor clusters in the inner galaxy.[4]
| Djorgovski 1 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Scorpius |
| Right ascension | 17h 47m 28.3s[1] |
| Declination | −33° 03:56′[1] |
| Distance | 44.7 kly[1] |
| Apparent magnitude (V) | 13.6[1] |
| Physical characteristics | |
| Metallicity | = −1.51[2] dex |
| Other designations | Djorg 1 |
![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c)
References edit
- ^ a b c d "Djorg 1". Spider.SEDS.org. Archived from the original on 4 March 2016. Retrieved 19 June 2015.
- ^ Valenti, Elena; Ferraro, Francesco R; Origlia, Livia. "Near-IR Properties of Globular Clusters in the Galactic Bulge". Archived from the original on 23 September 2015. Retrieved 19 June 2015.
- ^ Djorgovski, S (1987). "Discovery of three obscured globular clusters" (PDF). The Astrophysical Journal. 317: L13. Bibcode:1987ApJ...317L..13D. doi:10.1086/184903.
- ^ "Engulfed by stars near the Milky Way's heart". Hubble Space telescope. Archived from the original on 19 June 2015. Retrieved 19 June 2015.