NGC 908

{{Short description|Galaxy in the constellation Cetus}}

{{Infobox galaxy

| name = NGC 908

| image = NGC908.jpg

| caption = NGC 908 imaged by the Very Large Telescope of ESO.

| epoch = J2000

| type = SA(s)c {{cite web

| website=NASA/IPAC Extragalactic Database

| title=Results for NGC 908

| url=http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+908

| access-date=2006-11-18 }}

| ra = {{RA|02|23|04.6}}

| dec = {{DEC|-21|14|02}}

| dist_ly = 56.0 ± 5.7 Mly (17.2 ± 1.8 Mpc)

| z = 1509 ± 5 km/s

| appmag_v = 10.83

| size_v = 6′.0 × 2′.6

| constellation name = Cetus

| group_cluster = NGC 908 group

| notes =

| names = {{odlist|UGCA=27|PGC=9057|MCG=-04-06-035}}{{cite web|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+908&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|title=Your NED Search Results|website=NASA/IPAC Extragalactic Database|access-date=2020-11-09}}

}}

NGC 908 is an unbarred spiral galaxy in the constellation Cetus. It was discovered on 20 September 1786 by William Herschel.{{cite web | url = https://cseligman.com/text/atlas/ngc9.htm#908 | title = New General Catalogue Objects: NGC{{nbsp}}908 | last = Seligman | first = Courtney | website = Celestial Atlas | access-date = 29 August 2024 }} This galaxy is 56 million light years away from Earth. It is the main galaxy in the NGC 908 group, which also includes NGC 899, NGC 907, and IC 223.{{cite journal|last1=Dmitry Makarov and Igor Karachentsev|title=Galaxy groups and clouds in the local (z∼ 0.01) Universe|journal=MNRAS|date=2011|volume=412|issue=4|pages=2498–2520|doi=10.1111/j.1365-2966.2010.18071.x|doi-access=free |arxiv=1011.6277|bibcode=2011MNRAS.412.2498M|s2cid=119194025}}

Appearance

NGC 908 has vigorous star formation and is a starburst galaxy. The galaxy has a three-arm spiral pattern; two of its arms have peculiar morphology. The galaxy has a bright central bulge. Clusters of young stars and star-forming knots can be seen in the arms. Starburst activity and the peculiar morphology of the galaxy indicate it had a close encounter with another galaxy, although none are visible now.{{cite web|url=https://www.eso.org/public/images/eso0627a/|title=The Starburst Galaxy NGC 908|website=ESO|date=26 July 2006|access-date=9 November 2020}}

Stars observed

Two supernovae have been observed in NGC 908:

  • SN{{nbsp}}1994ai (type Ic, mag. 17) was discovered by Robert McNaught on 20 December 1994.{{cite journal | bibcode=1994IAUC.6120....1W| title=Supernova 1994ai in NGC 908| last1=Williams| first1=A.| last2=Martin| first2=R.| last3=Benetti| first3=S.| journal=International Astronomical Union Circular| date=1994| issue=6120| page=1}}{{cite web | website=Transient Name Server | title=SN{{nbsp}}1994ai | url=https://www.wis-tns.org/object/1994ai | publisher = IAU | access-date=22 August 2024}}
  • SN{{nbsp}}2006ce (type Ia, mag. 12.4) was discovered by Libert "Berto" Monard on 10 May 2006.{{cite journal | bibcode=2006IAUC.8709....1P| title=Supernovae 2006cb, 2006cc, 2006cd, 2006ce| last1=Ponticello| first1=N. J.| last2=Khandrika| first2=H.| last3=Madison| first3=D. R.| last4=Li| first4=W.| last5=Newton| first5=J.| last6=Crowley| first6=T.| last7=Puckett| first7=T.| last8=Monard| first8=L. A. G.| last9=Sehgal| first9=A.| journal=International Astronomical Union Circular| date=2006| issue=8709| page=1}}{{cite web | website=Transient Name Server | title=SN{{nbsp}}2006ce | url=https://www.wis-tns.org/object/2006ce | publisher = IAU | access-date=22 August 2024}}

Also, one luminous blue variable has been observed in this galaxy: AT 2021ablz (type LBV, mag. 20.6) was discovered by Pan-STARRS on 14 October 2021.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2021ablz | url=https://www.wis-tns.org/object/2021ablz | publisher = IAU | access-date=22 August 2024}}

See also

References

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