Astronomy:NGC 3125
From HandWiki
| NGC 3125 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Antlia |
| Right ascension | 10h 06m 33s |
| Declination | -29° 56’ 05” |
| Redshift | 0.003712 ± 0.000023 [1] |
| Helio radial velocity | 1113 ± 7 km/s[1] |
| Apparent magnitude (B) | 13.45 |
| Characteristics | |
| Type | S;BCDG [1] |
| Apparent size (V) | 1.1′ × 0.7′ |
| Other designations | |
| ESO 435-G041, AM 1004-294, MCG -05-24-022 | |
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.[2][3] It is located approximately 38 million light-years away from Earth.[4][5] Starburst galaxies are galaxies in which unusually high numbers of new stars are forming, springing to life within intensely hot clouds of gas.[6]
Morphology
In a 2006 study, the two giant H II regions in the galaxy were confirmed to each host two young star clusters.[2] The brightest cluster, NGC 3125-A1 is a confirmed super star cluster with 170,000 solar masses[7] that likely contains some of the most massive stars every found.[4][5]
Nearby galaxies
NGC 3125 is member of the LGG 189 Group, which also includes the galaxies NGC 3113, NGC 3137, and NGC 3175.[8]
See also
References
- ↑ 1.0 1.1 1.2 "NASA/IPAC Extragalactic Database". Results for NGC 3125. http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+3125.
- ↑ 2.0 2.1 Hadfield, L. J.; Crowther, P. A. (2006-06-01). "How extreme are the Wolf-Rayet clusters in NGC3125?*". Monthly Notices of the Royal Astronomical Society 368 (4): 1822–1832. doi:10.1111/j.1365-2966.2006.10245.x. ISSN 0035-8711. Bibcode: 2006MNRAS.368.1822H.
- ↑ "New General Catalog Objects: NGC 3100 - 3149". https://cseligman.com/text/atlas/ngc31.htm#3125.
- ↑ 4.0 4.1 Wofford, A.; Sixtos, A.; Smith, L.; Charlot, S.; Bruzual, G. (2024-01-01). "NGC 3125-A1 revisited at higher spectral resolution with COS G160M". IAU Symposium 361: 58–62. doi:10.1017/S1743921322002502. Bibcode: 2024IAUS..361...58W. https://ui.adsabs.harvard.edu/abs/2024IAUS..361...58W/abstract.
- ↑ 5.0 5.1 Plana, Henri; Alves, Vitor G.; Carvalho, Maiara S. (2024-06-01). "The influence of ionized gas kinematics on H II galaxies - the cases of Tol 1004-296 and Tol 0957-278". Monthly Notices of the Royal Astronomical Society 531 (2): 2881–2902. doi:10.1093/mnras/stae1327. ISSN 0035-8711. Bibcode: 2024MNRAS.531.2881P.
- ↑ Now, Astronomy. "NGC 3125 – Astronomy Now" (in en-US). https://astronomynow.com/tag/ngc-3125/.
- ↑ Wofford, Aida; Leitherer, Claus; Chandar, Rupali; Bouret, Jean-Claude (2014-02-01). "A Rare Encounter with Very Massive Stars in NGC 3125-A1". The Astrophysical Journal 781 (2): 122. doi:10.1088/0004-637X/781/2/122. ISSN 0004-637X. Bibcode: 2014ApJ...781..122W. https://ui.adsabs.harvard.edu/abs/2014ApJ...781..122W.
- ↑ Garcia, A. M. (1 July 1993). "General study of group membership. II. Determination of nearby groups.". Astronomy and Astrophysics Supplement Series 100: 47–90. ISSN 0365-0138. Bibcode: 1993A&AS..100...47G. https://cdsarc.cds.unistra.fr/ftp/J/A+AS/100/47/table2.dat.
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