NGC 376
{{short description|Globular cluster located in the constellation Tucana}}
{{Use mdy dates|date=November 2016}}
{{Infobox open cluster
| name = NGC 376
| image = NGC376 - HST - Potw2249a.jpg
| caption = Hubble Space Telescope image of NGC 376
| epoch = J2000
| constellation = Tucana
| dist_ly =
| size_v =
| mass_msol = {{Val|3400|400|fmt=commas}}
| age = {{Val|28|7}} Myr
| notes =
| names = ESO 029-SC 029.
}}
NGC 376 is a young open cluster of stars in the southern constellation of Tucana. It was discovered on September 2, 1826, by Scottish astronomer James Dunlop. Dreyer, a Danish/British astronomer, described it as a "globular cluster, bright, small, round." It is irregular in form, with a central spike.
The cluster is located in the eastern extension of the Small Magellanic Cloud (SMC), a nearby dwarf galaxy. It may have already lost 90% of its original mass and is in the process of dissolving into the SMC. As a result, it has achieved a relatively low concentration of stars and is no longer in dynamic equilibrium. The cluster is about 28 million years old and contains ~3,400 times the mass of the Sun. It has a core radius of {{Convert|2.34|±|0.10|pc|ly|1|disp=out|abbr=on}} and a tidal radius of {{Convert|5.88|±|0.20|pc|ly|1|disp=out|abbr=on}}.
References
{{reflist|refs=
| title=NGC 376
| access-date=2020-03-29 }}
| title=Is the Young Star Cluster NGC 376 Dissolving in the Field of the Small Magellanic Cloud?
| last1=Sabbi | first1=E. | last2=Nota | first2=A.
| last3=Tosi | first3=M. | last4=Smith | first4=L. J.
| last5=Gallagher | first5=J. | last6=Cignoni | first6=M.
| display-authors=1 | journal=The Astrophysical Journal
| volume=739 | issue=1 | id=15 | pages=10 | date=September 2011
| doi=10.1088/0004-637X/739/1/15 | arxiv=1106.5974
| bibcode=2011ApJ...739...15S | s2cid=115651242 }}
| title=The Star Clusters of the Small Magellanic Cloud: Age Distribution
| last1=Rafelski | first1=Marc | last2=Zaritsky | first2=Dennis
| journal=The Astronomical Journal
| volume=129 | issue=6 | pages=2701–2713 | date=June 2005
| doi=10.1086/424938 | arxiv=astro-ph/0408186
| bibcode=2005AJ....129.2701R | s2cid=4600017 }}
| title=Astrophysical properties of star clusters in the Magellanic Clouds homogeneously estimated by ASteCA
| display-authors=1 | last1=Perren | first1=G. I.
| last2=Piatti | first2=A. E. | last3=Vázquez | first3=R. A.
| journal=Astronomy & Astrophysics
| volume=602 | id=A89 | pages=42 | date=June 2017
| doi=10.1051/0004-6361/201629520 | arxiv=1701.08640
| bibcode=2017A&A...602A..89P | s2cid=56284363 }}
| title=New General Catalog Objects: NGC 350 - 399
| url=http://cseligman.com/text/atlas/ngc3.htm#376
| publisher=Cseligman | access-date=November 30, 2016 }}
}}
External links
- {{cite web
| title=NASA/IPAC Extragalactic Database
| work=Results for NGC 0376
| url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+376&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
| access-date=September 2, 2016}}
- {{commons category-inline}}
{{NGC5}}{{Tucana}}
{{DEFAULTSORT:NGC 376}}
Category:Small Magellanic Cloud
{{star-cluster-stub}}