NGC 3125

{{Infobox galaxy

|image=Extreme NGC 3125.png|name=NGC 3125

|ra=10h 06m 33s|dec=-29° 56’ 05”|epoch=J2000

|sbrightness=22.63 mag/arcsec2|appmag_b=13.45

|constellation name=Antlia

| names = ESO 435-G041, AM 1004-294, MCG -05-24-022

| size_v = 1.1{{prime}} × 0.7{{prime}}

| type = S;BCDG {{cite web

| title=NASA/IPAC Extragalactic Database

| work=Results for NGC 3125

| url=http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+3125

| access-date=2024-03-26 }}

| z = 0.003712 ± 0.000023

| h_radial_v = 1113 ± 7 km/s

}}

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

NGC 3125 is an irregular dwarf starburst galaxy in the constellation Antlia that was discovered by John Herschel in 1835.{{Cite journal |last1=Hadfield |first1=L. J. |last2=Crowther |first2=P. A. |date=2006-06-01 |title=How extreme are the Wolf-Rayet clusters in NGC3125?* |journal=Monthly Notices of the Royal Astronomical Society |volume=368 |issue=4 |pages=1822–1832 |doi=10.1111/j.1365-2966.2006.10245.x |doi-access=free |arxiv=astro-ph/0602591 |bibcode=2006MNRAS.368.1822H |issn=0035-8711}}{{Cite web |title=New General Catalog Objects: NGC 3100 - 3149 |url=https://cseligman.com/text/atlas/ngc31.htm#3125 |access-date=2025-02-16 |website=cseligman.com}} It is located approximately 38 million light-years away from Earth.{{Cite journal |last1=Wofford |first1=A. |last2=Sixtos |first2=A. |last3=Smith |first3=L. |last4=Charlot |first4=S. |last5=Bruzual |first5=G. |date=2024-01-01 |title=NGC 3125-A1 revisited at higher spectral resolution with COS G160M |journal=IAU Symposium |url=https://ui.adsabs.harvard.edu/abs/2024IAUS..361...58W/abstract |volume=361 |pages=58–62 |doi=10.1017/S1743921322002502|bibcode=2024IAUS..361...58W }}{{Cite journal |last1=Plana |first1=Henri |last2=Alves |first2=Vitor G. |last3=Carvalho |first3=Maiara S. |date=2024-06-01 |title=The influence of ionized gas kinematics on H II galaxies - the cases of Tol 1004-296 and Tol 0957-278 |journal=Monthly Notices of the Royal Astronomical Society |volume=531 |issue=2 |pages=2881–2902 |doi=10.1093/mnras/stae1327 |doi-access=free |arxiv=2405.12361 |bibcode=2024MNRAS.531.2881P |issn=0035-8711}} Starburst galaxies are galaxies in which unusually high numbers of new stars are forming, springing to life within intensely hot clouds of gas.{{Cite web |last=Now |first=Astronomy |title=NGC 3125 – Astronomy Now |url=https://astronomynow.com/tag/ngc-3125/ |access-date=2024-04-19 |language=en-US}}

Morphology

In a 2006 study, the two giant H II regions in the galaxy were confirmed to each host two young star clusters. The brightest cluster, NGC 3125-A1 is a confirmed super star cluster with 170,000 solar masses{{Cite journal |last1=Wofford |first1=Aida |last2=Leitherer |first2=Claus |last3=Chandar |first3=Rupali |last4=Bouret |first4=Jean-Claude |date=2014-02-01 |title=A Rare Encounter with Very Massive Stars in NGC 3125-A1 |url=https://ui.adsabs.harvard.edu/abs/2014ApJ...781..122W |journal=The Astrophysical Journal |volume=781 |issue=2 |pages=122 |arxiv=1312.5982 |doi=10.1088/0004-637X/781/2/122 |bibcode=2014ApJ...781..122W |issn=0004-637X}} that likely contains some of the most massive stars every found.

Nearby galaxies

NGC 3125 is member of the LGG 189 Group, which also includes the galaxies NGC 3113, NGC 3137, and NGC 3175.{{cite journal |last1=Garcia |first1=A. M. |title=General study of group membership. II. Determination of nearby groups. |journal=Astronomy and Astrophysics Supplement Series |date=1 July 1993 |volume=100 |pages=47–90 |url=https://cdsarc.cds.unistra.fr/ftp/J/A+AS/100/47/table2.dat |bibcode= 1993A&AS..100...47G |issn=0365-0138}}

See also

References