| NGC 6284 | |
|---|---|
 NGC 6284 as seen through the
Hubble Space Telescope | |
| Observation data ( J2000 epoch) | |
| Class | IX |
| Constellation | Ophiuchus |
| Right ascension | 17h 04m 28.747s [1] |
| Declination | −24° 45′ 51.22″ [1] |
| Distance | 43,000 ly [2] (13,200 pc [2]) |
| Apparent magnitude (V) | 7.43 [1] |
| Apparent dimensions (V) | 6.2' × 6.2' [3] |
| Physical characteristics | |
| Metallicity | = -1.26 [4] dex |
| Estimated age | 13.3~ billion years |
| Other designations | GCl 53, 2MASX J17042874-2445512 [1] |
![{\displaystyle {\begin{smallmatrix}\left[{\ce {Fe}}/{\ce {H}}\right]\end{smallmatrix}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/4c0821bd80891e071c08e7c7ee8e022baedf522c)
NGC 6284 is a globular cluster located in the constellation Ophiuchus. It is designated as IX in the galaxy morphological classification scheme and was discovered by the German-born British astronomer William Herschel on 22 May 1784. Its distance had previously been estimated at 49,900 light years from Earth, [5] [3] [6] [7] [8] but this was revised in 2023 to around 43,000 light years. [2] This same study, based on high-resolution Hubble Space Telescope optical observations, produced the first high-quality colour-magnitude diagram (CMD) of NGC 6284, extending down to about six magnitudes below its main sequence turn-off. The new observations moved its centre of gravity by 1.5–3 arcseconds from previous values, and its density profile showed a steep central cusp, suggesting that NGC 6284 is a post-core collapse (PCC) cluster.
The nearby metal-poor star HD 194598 may be a recent runaway from NGC 6284. [9]
See also
References
- ^ a b c d "NGC 6284". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c "Globular cluster NGC 6284 inspected by astronomers".
- ^ a b "Revised NGC Data for NGC 6284". Seds. Retrieved 3 October 2015.
- ^ William E. Harris. "Catalog of Parameters for Milky Way Globular Clusters". Retrieved 3 February 2017.
- ^ "Object No. 1 - NGC 6284". NASA/IPAC extragalactic database. NASA/IPAC. Retrieved 3 October 2015.
- ^ "NGC 6284 (= GCL 53)". cseligman. Retrieved 3 October 2015.
- ^ "NGC 6284". Seds. Retrieved 3 October 2015.
- ^ "The globular cluster NGC 6284". In-the-sky. Retrieved 3 October 2015.
- ^ Şahin, Timur; Bilir, Selçuk (2020), "On the Origin of Metal-poor Stars in the Solar Neighborhood", The Astrophysical Journal, 899 (1): 41, arXiv: 2007.08514, Bibcode: 2020ApJ...899...41S, doi: 10.3847/1538-4357/aba2d2, S2CID 220545932
External links
-
Media related to
NGC 6284 at Wikimedia Commons
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |
| NGC 6284 | |
|---|---|
|
NGC 6284 as seen through the
Hubble Space Telescope | |
| Observation data ( J2000 epoch) | |
| Class | IX |
| Constellation | Ophiuchus |
| Right ascension | 17h 04m 28.747s [1] |
| Declination | −24° 45′ 51.22″ [1] |
| Distance | 43,000 ly [2] (13,200 pc [2]) |
| Apparent magnitude (V) | 7.43 [1] |
| Apparent dimensions (V) | 6.2' × 6.2' [3] |
| Physical characteristics | |
| Metallicity | = -1.26 [4] dex |
| Estimated age | 13.3~ billion years |
| Other designations | GCl 53, 2MASX J17042874-2445512 [1] |
NGC 6284 is a globular cluster located in the constellation Ophiuchus. It is designated as IX in the galaxy morphological classification scheme and was discovered by the German-born British astronomer William Herschel on 22 May 1784. Its distance had previously been estimated at 49,900 light years from Earth, [5] [3] [6] [7] [8] but this was revised in 2023 to around 43,000 light years. [2] This same study, based on high-resolution Hubble Space Telescope optical observations, produced the first high-quality colour-magnitude diagram (CMD) of NGC 6284, extending down to about six magnitudes below its main sequence turn-off. The new observations moved its centre of gravity by 1.5–3 arcseconds from previous values, and its density profile showed a steep central cusp, suggesting that NGC 6284 is a post-core collapse (PCC) cluster.
The nearby metal-poor star HD 194598 may be a recent runaway from NGC 6284. [9]
See also
References
- ^ a b c d "NGC 6284". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b c "Globular cluster NGC 6284 inspected by astronomers".
- ^ a b "Revised NGC Data for NGC 6284". Seds. Retrieved 3 October 2015.
- ^ William E. Harris. "Catalog of Parameters for Milky Way Globular Clusters". Retrieved 3 February 2017.
- ^ "Object No. 1 - NGC 6284". NASA/IPAC extragalactic database. NASA/IPAC. Retrieved 3 October 2015.
- ^ "NGC 6284 (= GCL 53)". cseligman. Retrieved 3 October 2015.
- ^ "NGC 6284". Seds. Retrieved 3 October 2015.
- ^ "The globular cluster NGC 6284". In-the-sky. Retrieved 3 October 2015.
- ^ Şahin, Timur; Bilir, Selçuk (2020), "On the Origin of Metal-poor Stars in the Solar Neighborhood", The Astrophysical Journal, 899 (1): 41, arXiv: 2007.08514, Bibcode: 2020ApJ...899...41S, doi: 10.3847/1538-4357/aba2d2, S2CID 220545932
External links
-
Media related to
NGC 6284 at Wikimedia Commons
|
| This star cluster–related article is a stub. You can help Wikipedia by expanding it. |