NGC 371

{{short description|Open cluster in the constellation Tucana}}

{{Infobox galaxy

| name = NGC 371

| image = NGC 371.jpg

| caption = NGC 371 image using the FORS1 instrument on ESO’s Very Large Telescope

| epoch = J2000

| constellation name = Tucana

| ra = {{RA|01|03|25}} {{cite simbad

| title=NGC 371

| access-date=2010-03-31}}

| dec = {{DEC|-72|04.4|00}}

| z =

| h_radial_v =

| dist_ly = 200000 ly (61320 pc)

| type =

| appmag_v =

| size_v =

| notes =

| names = Cl Kron 48, ESO 51-14, Cl Lindsay 71, Cl Melotte 5

}}

NGC 371, also called Hodge 53, is an open cluster 200,000 light-years (61,320 pc) away located in the Small Magellanic Cloud in Tucana constellation. It was discovered on 1 August 1826 by Scottish astronomer James Dunlop.{{cite web | url = https://cseligman.com/text/atlas/ngc3a.htm#371 | title = New General Catalogue Objects: NGC{{nbsp}}371 | last = Seligman | first = Courtney | website = Celestial Atlas | access-date = 29 August 2024 }}

class="wikitable sortable"

|+Prominent stars{{Cite journal|last1=Massey|first1=Philip|last2=Waterhouse|first2=Elizabeth|last3=DeGioia-Eastwood|first3=Kathleen|author3-link=Kathy Eastwood|date=May 2000|title=The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. I. Results from 19 OB Associations in the Magellanic Clouds|url=https://iopscience.iop.org/article/10.1086/301345|journal=The Astronomical Journal|volume=119|issue=5|pages=2214–2241|arxiv=astro-ph/0002233|bibcode=2000AJ....119.2214M|doi=10.1086/301345|issn=0004-6256|s2cid=16891188}}{{cite journal|bibcode=2016A&A...591A..22S|title=Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries|volume=1604|arxiv=1604.01022|last1=Shenar|first1=T.|last2=Hainich|first2=R.|last3=Todt|first3=H.|last4=Sander|first4=A.|last5=Hamann|first5=W.-R.|last6=Moffat|first6=A. F. J.|last7=Eldridge|first7=J. J.|last8=Pablo|first8=H.|last9=Oskinova|first9=L. M.|last10=Richardson|first10=N. D.|year=2016|doi=10.1051/0004-6361/201527916|journal=Astronomy & Astrophysics|page=A22|s2cid=119255408 }}

!Star name

!Effective temperature (K)

!Absolute magnitude

!Bolometric magnitude

!Mass ({{solar mass|link=yes}})

!Spectral type

AB6

|105000/35000

| -5.15/-6.65

| -10.96/-10.01

|9/41

|WN4+O6.5I

AB7

|105000/36000

| -4.4/-5.7

| -10.51/-9.01

|23/44

|WN4+O6I(f)

Hodge53-207

|50100

| -4.8

| -9.3

|53

|O

Hodge53-47a

|48600

| -4.9

| -9.3

|50

|O4V

Hodge53-47b

|42400

| -4.9

| -8.9

|37

|O6.5V

Hodge53-60

|37200

| -5.4

| -9

|36

|O8III

AV 327

|33000

| -5.8

| -9.1

|35

|O9I

Hodge53-141

|34400

| -5.8

| -9.2

|34

|O9III

Hodge53-137

|35700

| -5.6

| -9.1

|34

|O8.5III

Hodge53-118

|42500

| -4.6

| -8.6

|34

|

Hodge53-91

|37200

| -5.1

| -8.7

|32

|O8.5V

Hodge53-11

|41800

| -4.4

| -8.3

|31

|

Hodge53-74

|39400

| -4.6

| -8.4

|30

|

See also

References

{{Reflist}}