NGC 6355: Difference between revisions
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| pronounce = |
| pronounce = |
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| constellation = [[Ophiuchus]] |
| constellation = [[Ophiuchus]] |
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⚫ | | ra = {{RA|17|23|58.6}}<ref name="NASA/IPAC">{{cite web|title=Object No. 1 - NGC 6355|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+6355&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=14 October 2015}}</ref><ref name=Seds>{{cite web|title=Revised NGC Data for NGC 6355|url=http://spider.seds.org/ngc/revngcic.cgi?NGC6355|website=Seds|access-date=14 October 2015}}</ref> |
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| ra = {{RA|17|23|58.6}} <!-- or {{Deg2HMS|000.0000|sup=yes}} --> |
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| dec = {{DEC|-26|21|12}} |
| dec = {{DEC|-26|21|12}}<ref name="NASA/IPAC"/> |
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| z = <!--{{val||}}--> |
| z = <!--{{val||}}--> |
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| h_radial_v = {{val|-176.9|7.1|u=km/s}} |
| h_radial_v = {{val|-176.9|7.1|u=km/s}} |
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| gal_v = <!--{{val|||u=km/s}}--> |
| gal_v = <!--{{val|||u=km/s}}--> |
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| dist_pc = |
| dist_pc = {{convert|8.54|+/-|0.19|kpc|kly|abbr=on|lk=on}}<ref name=Souza/> |
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| dist_ly = <!--{{convert|000|+/-|00|kly|kpc|abbr=on|lk=on}}{{hub|0.73}}--> |
| dist_ly = <!--{{convert|000|+/-|00|kly|kpc|abbr=on|lk=on}}{{hub|0.73}}--> |
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| group_cluster = |
| group_cluster = |
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| type = |
| type = |
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| mass = <!-- In solar masses --> <!--{{Val|0|e=0}}--> |
| mass = <!-- In solar masses --> <!--{{Val|0|e=0}}--> |
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| mass_light_ratio = <!-- In solar units --> |
| mass_light_ratio = <!-- In solar units --> |
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| size = <!-- In light years --> |
| size = <!-- In light years --> |
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| stars = |
| stars = |
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| age = 13.2 ± 1.1 Gyr<ref name=Souza>{{cite journal|doi=10.1051/0004-6361/202245286 |title=Chrono-chemodynamical analysis of the globular cluster NGC 6355: Looking for the fundamental bricks of the Bulge |date=2023 |last1=Souza |first1=S. O. |last2=Ernandes |first2=H. |last3=Valentini |first3=M. |last4=Barbuy |first4=B. |last5=Chiappini |first5=C. |last6=Pérez-Villegas |first6=A. |last7=Ortolani |first7=S. |last8=Friaça |first8=A. C. S. |last9=Queiroz |first9=A. B. A. |last10=Bica |first10=E. |journal=Astronomy & Astrophysics |volume=671 |pages=A45 |bibcode=2023A&A...671A..45S | arxiv=2301.05227 }}</ref> |
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| appmag_v = 8.6 |
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| metal_fe = −1.39 ± 0.08<ref name=Souza/> |
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| appmag_v = 8.6<ref name=Seds1>{{cite web|title=NGC 6355|url=http://spider.seds.org/spider/MWGC/n6355.html|website=Seds|access-date=14 October 2015}}</ref> |
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| absmag_v = -8.07 |
| absmag_v = -8.07 |
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| size_v = 4.20 |
| size_v = 4.20<ref name=Seds1/> |
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| notes = |
| notes = |
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| names = [[Collinder catalogue|Cr]] 330, GCL 63 and ESO 519-SC15 |
| names = [[Collinder catalogue|Cr]] 330, GCL 63 and ESO 519-SC15 |
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| references = |
| references = |
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}} |
}} |
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'''NGC 6355''' is a [[globular cluster]] located in the constellation [[Ophiuchus]].<ref name=In-the-sky>{{cite web|title=The globular cluster NGC 6355|url=https://in-the-sky.org/data/object.php?id=NGC6355|website=In-the-sky|access-date=31 October 2016}}</ref> It is at a distance of 28,000 light years away from Earth, and is currently part of the [[Galactic bulge]].<ref name=Souza/> |
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NGC was discovered by the German-born British astronomer [[William Herschel]] on 24 May 1784.<ref name=cseligman>{{cite web|title=NGC 6355 (= GCL 63)|url=http://cseligman.com/text/atlas/ngc63a.htm#6355|website=cseligman|access-date=14 October 2015}}</ref> It was initially thought to be an [[open cluster]], but its true nature as a globular cluster was later confirmed. It is a [[core collapse (cluster)|core-collapse]] cluster.<ref name=Souza/> |
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== See also == |
== See also == |
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{{Astronomical catalogs|NGC=6355|Collinder=330}} |
{{Astronomical catalogs|NGC=6355|Collinder=330}} |
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{{NGC objects:6000-6499}} |
{{NGC objects:6000-6499}} |
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{{Ophiuchus}} |
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[[Category:Globular clusters]] |
[[Category:Globular clusters]] |
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[[Category:NGC objects|6355]] |
[[Category:NGC objects|6355]] |
Latest revision as of 18:14, 1 December 2024
NGC 6355 | |
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Observation data (J2000 epoch) | |
Constellation | Ophiuchus |
Right ascension | 17h 23m 58.6s[1][2] |
Declination | −26° 21′ 12″[1] |
Distance | 8.54 ± 0.19 kpc (27.85 ± 0.62 kly)[3] |
Apparent magnitude (V) | 8.6[4] |
Apparent dimensions (V) | 4.20[4] |
Physical characteristics | |
Absolute magnitude | -8.07 |
Metallicity | = −1.39 ± 0.08[3] dex |
Estimated age | 13.2 ± 1.1 Gyr[3] |
Other designations | Cr 330, GCL 63 and ESO 519-SC15 |
NGC 6355 is a globular cluster located in the constellation Ophiuchus.[5] It is at a distance of 28,000 light years away from Earth, and is currently part of the Galactic bulge.[3]
NGC was discovered by the German-born British astronomer William Herschel on 24 May 1784.[6] It was initially thought to be an open cluster, but its true nature as a globular cluster was later confirmed. It is a core-collapse cluster.[3]
See also
[edit]References
[edit]- ^ a b "Object No. 1 - NGC 6355". NASA/IPAC extragalactic database. NASA/IPAC. Retrieved 14 October 2015.
- ^ "Revised NGC Data for NGC 6355". Seds. Retrieved 14 October 2015.
- ^ a b c d e Souza, S. O.; Ernandes, H.; Valentini, M.; Barbuy, B.; Chiappini, C.; Pérez-Villegas, A.; Ortolani, S.; Friaça, A. C. S.; Queiroz, A. B. A.; Bica, E. (2023). "Chrono-chemodynamical analysis of the globular cluster NGC 6355: Looking for the fundamental bricks of the Bulge". Astronomy & Astrophysics. 671: A45. arXiv:2301.05227. Bibcode:2023A&A...671A..45S. doi:10.1051/0004-6361/202245286.
- ^ a b "NGC 6355". Seds. Retrieved 14 October 2015.
- ^ "The globular cluster NGC 6355". In-the-sky. Retrieved 31 October 2016.
- ^ "NGC 6355 (= GCL 63)". cseligman. Retrieved 14 October 2015.
External links
[edit]- Media related to NGC 6355 at Wikimedia Commons