NGC 7619

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

{{Infobox galaxy

| name = NGC 7619

| image = 250px

| alt = NGC 7619

| caption = SDSS image of NGC 7619

| constellation name = Pegasus

| epoch = J2000

| ra = {{RA|23|17|14.524}}{{cite web |url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC+7619 |title=NGC 7619 |author= |website=Simbad |publisher=Université de Strasbourg/CNRS |access-date=2021-02-10 }}

| dec = {{DEC|+08|12|22.63}}

| h_radial_v = 3,944 km/s

| z = 0.01324

| appmag_b = 12.7

| type = E2

| names = {{odlist|UGC=12523|MCG=+01-59-052|PGC=71121}}

}}

NGC 7619 is an elliptical galaxy located in the constellation Pegasus. NGC 7619 and NGC 7626 are the dominant and brightest members of the Pegasus galaxy cluster. Both of them were discovered by William Herschel on September 26, 1785.{{cite web|url=http://cseligman.com/text/atlas/ngc76.htm#7619|title=New General Catalogue objects: NGC 7600 - 7649|author=Seligman, Courtney|website=cseligman.com|accessdate=2021-02-10}}

The radial velocity of this galaxy was measured in 1929 and found to be double that of any galaxy observed at that time. The measurement was consistent with the extrapolated value predicted by Edwin Hubble; a distance-velocity relation that would later become known as Hubble's law.

One supernova has been observed in NGC 7619: SN 1970J (type Ia, mag. 14.5) was discovered by Leonida Rosino on 24 September 1970.{{cite web | website=Transient Name Server | title=SN{{nbsp}}1970J | url=https://www.wis-tns.org/object/1970J | publisher = IAU | access-date=2 December 2024}}{{cite simbad|title= SN 1970J|accessdate=2021-02-10}}

References

{{reflist|refs=

{{Cite journal |last=Hodge |first=Paul W. |date=1961-07-01 |title=The Gravitattional Stability of the NGC 7619 Group of Galaxies. |journal=The Astrophysical Journal |volume=134 |pages=262 |doi=10.1086/147151|bibcode=1961ApJ...134..262H |doi-access=free }}

{{Cite journal |last1=Randall |first1=S. W. |last2=Jones |first2=C. |last3=Kraft |first3=R. |last4=Forman |first4=W. R. |last5=Sullivan |first5=E. |date=April 2009 |title=Merging Cold Fronts In The Galaxy Pair NGC 7619 AND NGC 7626 |journal=The Astrophysical Journal |volume=696 |issue=2 |pages=1431–1440 |language=en |doi=10.1088/0004-637X/696/2/1431|arxiv=0811.1217 |bibcode=2009ApJ...696.1431R |s2cid=14950971 |doi-access=free }}

{{cite journal |doi=10.1073/pnas.27.8.366|title=Remarks on the Pegasus Cluster of Nebulae|year=1941|last1=Edson|first1=J. B.|last2=Zwicky|first2=F.|journal=Proceedings of the National Academy of Sciences|volume=27|issue=8|pages=366–369|pmid=16588471|pmc=1078341|bibcode=1941PNAS...27..366E|doi-access=free }}

{{cite journal |last=Humason |first=Milton L. |date=March 15, 1929 |title=The Large Radial Velocity of N.G.C. 7619 |journal=PNAS |volume=15 |issue=3 |pages=167–168 |doi=10.1073/pnas.15.3.167 |pmid=16577159 |pmc=522426 |bibcode=1929PNAS...15..167H |doi-access=free }}

{{cite journal |last=Hubble |first=E.P. |title=A Clue to the Structure of the Universe |journal= Leaflet of the Astronomical Society of the Pacific|year=1929 |volume= 1|issue= 23|page=93 |bibcode=1929ASPL....1...93H }}

}}