NGC 958

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

{{Use dmy dates|date=November 2024}}

{{Sky|02|30|42.8350|-|02|56|20.126}}

{{Infobox Galaxy

| name = NGC 958

| image = NGC958 - SDSS DR14.jpg

| caption = NGC 958 imaged by SDSS

| constellation name = Cetus

| epoch = J2000

| type = SB(rs)c?{{cite web

| website = NASA/IPAC Extragalactic Database

| publisher = NASA and Caltech

| title = Results for object NGC 958

| url = https://ned.ipac.caltech.edu/byname?objname=NGC+958

| access-date = 10 August 2024}}

| ra = {{RA|02|30|42.8350}}

| dec = {{DEC|-02|56|20.126}}

| dist_ly = {{convert|81.20 ± 5.69|Mpc|Mly|abbr=on|lk=on|order=flip}}

| z = 0.019150

| h_radial_v = 5741 ± 2 km/s

| appmag_v = 12.2

| size_v = {{Val|2.9|×|0.9|u=arcminute}}{{r|ned}}

| size = ~{{convert|49.43|kpc|ly|abbr=on|lk=on|order=flip}} (estimated)

| names = {{odlist | PGC= 9560 | MCG= -01-07-019 | IRAS= 02281-0309 | 2MASX= J02304283-0256204}}

}}

NGC 958 is a barred spiral galaxy in the constellation of Cetus. Its velocity with respect to the cosmic microwave background is 5505 ± 17 km/s, which corresponds to a Hubble distance of 81.20 ± 5.69 Mpc (~265 million light-years). However, 19 non-redshift measurements give a closer distance of 58.93 ± 12.91 Mpc (~192 million light-years).{{cite web | url = https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+958 | title = Distance Results for NGC 958 | website = NASA/IPAC EXTRAGALACTIC DATABASE | publisher = NASA | access-date = 10 August 2024}} The galaxy was discovered by German-British astronomer William Herschel on 20 September 1784.{{cite web | url = https://cseligman.com/text/atlas/ngc9a.htm#958 | title = NGC 958 | last = Seligman | first = Courtney | website = Celestial Atlas | access-date = 10 August 2024 }}

The SIMBAD database lists NGC 958 as a Seyfert II Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.{{cite simbad | title=NGC 958 | access-date=16 December 2024}} The NASA/IPAC Extragalactic Database (NED) lists NGC 958 as a luminous infrared galaxy (LIRG).

Supernovae

Three supernovae have been observed in NGC 958:

  • SN 2005A (Type Ia, mag. 17.1) was discovered by the Lick Observatory Supernova Search (LOSS) on 5 January 2005.{{cite journal|bibcode=2005IAUC.8459....3G |title=Supernova 2005A in NGC 958 |last1=Graham |first1=J. |last2=Li |first2=W. |journal=International Astronomical Union Circular |date=2005 |issue=8459 |page=3 | url=http://www.cbat.eps.harvard.edu/iauc/08400/08459.html#Item2}}{{cite web | website=Transient Name Server | title=SN{{nbsp}}2005A | url=https://www.wis-tns.org/object/2005A | publisher = IAU | access-date=16 December 2024}}
  • SN 2022ao (Type Ic, mag. 17.997) was discovered by ATLAS on 5 January 2022.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2022ao | url=https://www.wis-tns.org/object/2022ao | publisher = IAU | access-date=16 December 2024}}
  • SN 2022acbu (Type II, mag. 20.34) was discovered by the Zwicky Transient Facility on 30 November 2022.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2022acbu | url=https://www.wis-tns.org/object/2022acbu | publisher = IAU | access-date=16 December 2024}}

See also

References

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