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

| ra = {{RA|01|03|50.21}}

| dec = {{DEC|-72|49|33.5}}

| dist_ly =

| appmag_v = 10.90

| 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=

{{cite simbad

| title=NGC 376

| access-date=2020-03-29 }}

{{cite journal

| 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 }}

{{cite journal

| 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 }}

{{cite journal

| 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 }}

{{cite web

| title=New General Catalog Objects: NGC 350 - 399

| url=http://cseligman.com/text/atlas/ngc3.htm#376

| publisher=Cseligman | access-date=November 30, 2016 }}

}}