NGC 6284: Difference between revisions
m Task 18b (cosmetic): eval 1 template: hyphenate params (1×); |
Entranced98 (talk | contribs) Adding local short description: "Globular cluster in the constellation Ophiuchus", overriding Wikidata description "globular cluster" |
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{{Short description|Globular cluster in the constellation Ophiuchus}} |
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{{Infobox globular cluster |
{{Infobox globular cluster |
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| name = NGC 6284 |
| name = NGC 6284 |
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| image = |
| image = File:NGC 6284 WFC3.jpg |
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| caption = NGC 6284 as seen through the [[Hubble Space Telescope]] |
| caption = NGC 6284 as seen through the [[Hubble Space Telescope]] |
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| credit = |
| credit = |
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| epoch = [[J2000]] |
| epoch = [[J2000]] |
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| class = IX |
| class = IX |
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| ra = {{RA|17|04|28.747}}<ref name=SIMBAD>{{cite simbad|title=NGC 6284|access-date 3 February 2017}}</ref> |
| ra = {{RA|17|04|28.747}}<ref name=SIMBAD>{{cite simbad|title=NGC 6284|access-date 3 February 2017}}</ref> |
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| dec = {{DEC|-24|45|51.22}}<ref name=SIMBAD/> |
| dec = {{DEC|-24|45|51.22}}<ref name=SIMBAD/> |
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| dist_ly = 43,000 ly<ref name="phys.org">{{cite web | url=https://phys.org/news/2023-11-globular-cluster-ngc-astronomers.html | title=Globular cluster NGC 6284 inspected by astronomers }}</ref> |
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| dist_ly = 49900 ly<ref name=Seds1/> |
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| dist_pc = 13,200 pc<ref name="phys.org">{{cite web | url=https://phys.org/news/2023-11-globular-cluster-ngc-astronomers.html | title=Globular cluster NGC 6284 inspected by astronomers }}</ref> |
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| dist_pc = 15300 pc<ref name=Seds1/> |
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| appmag_v = 7.43<ref name=SIMBAD/> |
| appmag_v = 7.43<ref name=SIMBAD/> |
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| size_v = 6.2' |
| size_v = 6.2' × 6.2'<ref name=Seds/> |
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| mass_msol = |
| mass_msol = |
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| mass_kg = |
| mass_kg = |
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| metal_fe = -1.26<ref>{{cite web|title=Catalog of Parameters for Milky Way Globular Clusters|url=http://physwww.mcmaster.ca/~harris/mwgc.dat|author1=William E. Harris|access-date=3 February 2017}}</ref> |
| metal_fe = -1.26<ref>{{cite web|title=Catalog of Parameters for Milky Way Globular Clusters|url=http://physwww.mcmaster.ca/~harris/mwgc.dat|author1=William E. Harris|access-date=3 February 2017}}</ref> |
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| metal_z = |
| metal_z = |
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| age = |
| age =13.3~ billion years |
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| notes = |
| notes = |
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| names = GCl 53, [[2MASX]] J17042874-2445512<ref name=SIMBAD/> |
| names = GCl 53, [[2MASX]] J17042874-2445512<ref name=SIMBAD/> |
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|image size=250}} |
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}} |
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'''NGC 6284''' is a [[globular cluster]] located in the constellation [[Ophiuchus]]. It is designated as '''IX''' in the [[Galaxy morphological classification|galaxy morphological classification scheme]] and was discovered by the German-born British astronomer [[William Herschel]] on 22 May 1784. |
'''NGC 6284''' is a [[globular cluster]] located in the constellation [[Ophiuchus]]. It is designated as '''IX''' in the [[Galaxy morphological classification|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,<ref name="NASA/IPAC">{{cite web|title=Object No. 1 - NGC 6284|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+6284&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|website=NASA/IPAC extragalactic database|publisher=NASA/IPAC|access-date=3 October 2015}}</ref><ref name=Seds>{{cite web|title=Revised NGC Data for NGC 6284|url=http://spider.seds.org/ngc/revngcic.cgi?NGC6284|website=Seds|access-date=3 October 2015}}</ref><ref name=cseligman>{{cite web|title=NGC 6284 (= GCL 53)|url=http://cseligman.com/text/atlas/ngc62a.htm#6284|website=cseligman|access-date=3 October 2015}}</ref><ref name=Seds1>{{cite web|title=NGC 6284|url=http://spider.seds.org/spider/MWGC/n6284.html|website=Seds|access-date=3 October 2015}}</ref><ref name=In-the-sky>{{cite web|title=The globular cluster NGC 6284|url=https://in-the-sky.org/data/object.php?id=5051|website=In-the-sky|access-date=3 October 2015}}</ref> but this was revised in 2023 to around 43,000 light years.<ref name="phys.org">{{cite web | url=https://phys.org/news/2023-11-globular-cluster-ngc-astronomers.html | title=Globular cluster NGC 6284 inspected by astronomers }}</ref> 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. |
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The nearby metal-poor star {{ill|HD 194598|es|HD 194598}} may be a recent [[Runaway star|runaway]] from NGC 6284.<ref>{{citation|arxiv=2007.08514|year=2020|title=On the Origin of Metal-poor Stars in the Solar Neighborhood|doi=10.3847/1538-4357/aba2d2 |last1=Şahin |first1=Timur |last2=Bilir |first2=Selçuk |journal=The Astrophysical Journal |volume=899 |issue=1 |page=41 |bibcode=2020ApJ...899...41S |s2cid=220545932 |doi-access=free }}</ref> |
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== See also == |
== See also == |
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== External links == |
== External links == |
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* {{ |
* {{commons category-inline}} |
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{{NGC objects:6000-6499}} |
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{{Ngc65}} |
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⚫ | |||
[[Category:Globular clusters]] |
[[Category:Globular clusters]] |
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[[Category:NGC objects|6284]] |
[[Category:NGC objects|6284]] |
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[[Category:Ophiuchus |
[[Category:Ophiuchus]] |
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⚫ |
Latest revision as of 22:42, 23 July 2024
NGC 6284 | |
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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
[edit]References
[edit]- ^ 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
[edit]- Media related to NGC 6284 at Wikimedia Commons