NGC 7769

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

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

{{Sky|23|51|03.9592|+|20|09|01.508}}

{{Infobox Galaxy

| name = NGC 7769

| image = NGC7769 - SDSS DR14.jpg

| caption= The spiral galaxy NGC 7769

| constellation name = Pegasus

| epoch = J2000

| type = (R)SA(rs)b{{cite web

| website=NASA/IPAC Extragalactic Database

| publisher = NASA and Caltech

| title=Results for object NGC 7769

| url=https://ned.ipac.caltech.edu/byname?objname=NGC+7769

| access-date=2 August 2024}}

| ra = {{RA|23|51|03.9592}}

| dec = {{DEC|+20|09|01.508}}

| dist_ly = {{convert|56.85 ± 4.00|Mpc|Mly|abbr=on|lk=on|order=flip}}

| group_cluster = NGC 7771 Group (LGG 483)

| z = 0.014046

| h_radial_v = 4211 ± 2 km/s

| appmag_v = 12.0

| size_v = {{Val|3.2|×|2.7|u=arcminute}}

| size = ~{{convert|54.14|kpc|ly|abbr=on|lk=on|order=flip}} (estimated)

| names = {{odlist | MRK= 9005 |name= HOLM 820C | PGC= 72615 | UGC= 12808 | CGCG= 455-054 | MCG= +03-60-030 | IRAS= 23485+1952 | 2MASX= J23510396+2009014}}

}}

NGC 7769 is an unbarred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 3855 ± 25 km/s, which corresponds to a Hubble distance of 56.85 ± 4 Mpc (~185 million light-years). It was discovered by German-British astronomer William Herschel on 18 September 1784.{{cite web | url = https://cseligman.com/text/atlas/ngc77a.htm#7769 | title = New General Catalogue Objects: NGC{{nbsp}}7769 | last = Seligman | first = Courtney | website = Celestial Atlas | access-date = 15 December 2024}}

The galaxies NGC 7769, together with NGC 7770 and NGC 7771, are listed together as Holm 820 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.{{cite journal | bibcode=1937AnLun...6....1H | title=A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems | last1=Holmberg | first1=Erik | journal=Annals of the Observatory of Lund | date=1937 | volume=6 | page=1}} NGC 7769 also is listed as part of the five-member NGC 7771 Group (also known as LGG 483), which contains the 3 galaxies from Holm 820, NGC 7786, and UGC 12828.{{cite journal | bibcode=1993A&AS..100...47G | title=General study of group membership. II. Determination of nearby groups | last1=Garcia | first1=A. M. | journal=Astronomy and Astrophysics Supplement Series | date=1993 | volume=100 | page=47}}

NGC 7769 is a LINER galaxy, i.e. it has a type of nucleus that is defined by its spectral line emission which has weakly ionized or neutral atoms, while the spectral line emission from strongly ionized atoms is relatively weak.

Supernovae

Three supernovae have been observed in NGC 7769:

  • SN 2019iex (type II, mag. 17.6) was discovered by the Searches After Gravitational-waves using ARizona Observatories (SAGUARO) project on 26 June 2019.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2019iex | url=https://www.wis-tns.org/object/2019iex | publisher = IAU | access-date=15 December 2024}}
  • SN 2022mxv (type II, mag. 18.249) was discovered by ATLAS on 18 June 2022.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2022mxv | url=https://www.wis-tns.org/object/2022mxv | publisher = IAU | access-date=13 January 2025}}
  • SN 2024grb (type II, mag. 18.2) was discovered by ATLAS on 16 April 2024.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2024grb | url=https://www.wis-tns.org/object/2024grb | publisher = IAU | access-date=15 December 2024}}

See also

References

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