| NGC 4298 | |
|---|---|
 Hubble Space Telescope image of NGC 4298 | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 21m 32.7s[1] |
| Declination | 14° 36′ 22″[1] |
| Redshift | 0.003786[1] |
| Heliocentric radial velocity | 1135 km/s[1] |
| Distance | 53 Mly (16.4 Mpc)[1] |
| Group or cluster | Virgo Cluster |
| Apparent magnitude (V) | 12.5[1] |
| Characteristics | |
| Type | SA(rs)c[1] |
| Mass | 1.5×1010[2] M☉ |
| Size | ~55,000 ly (17 kpc) (estimated)[1] |
| Apparent size (V) | 3.30 x 1.24[1] |
| Other designations | |
| CGCG 99-24, IRAS 12190+1452, KCPG 332A, MCG 3-32-7, PGC 39950, UGC 7412, VCC 483[1] | |
NGC 4298 is a flocculent[3][4][5][6] spiral galaxy located about 53 million light-years away[7] in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 8, 1784[8] and is a member of the Virgo Cluster.[9][10][11]
NGC 4298 may harbor an intermediate-mass black hole with an estimated mass ranging from 20,000 (2×104 M☉) to 500,000 (5×105 M☉) solar masses.[12]
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Zoom-in on NGC 4298 and NGC 4302
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Pan on NGC 4298 and NGC 4302
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Classroom Aid - NGC 4302 & 4298
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Hubble captured stunning Virgo galaxy cluster : NGC 4302 and NGC 4298
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Fulldome view of NGC 4298 and NGC 4302
Transcription
Interaction with NGC 4302
NGC 4298 appears to form a pair with[13][14][15] and appears to interact with NGC 4302.[13][2][14][16][15][17][18][4] Evidence for an interaction between the two galaxies are that NGC 4298 exhibits a lopsided, asymmetrical distribution of stars,[4][16][15] a tidal bridge that connects it to NGC 4302,[18][17][2] a prodigious rate of star formation[19] and an HI-tail. However, the tail is also the result of ram pressure.[3]
The two galaxies are separated from a projected distance of ~36,000 ly (11 kpc).[20][15][3]
Ram-pressure stripping
The presence of a truncated gas disc,[3][4] an asymmetric 6 cm polarized radio continuum distribution,[13] an HI-tail,[3] and asymmetries of gas in a similar direction as the ram pressure stripped gas in NGC 4302 suggest that NGC 4298 is under going ram pressure.[2]
See also
References
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 4298. Retrieved 2019-03-02.
- ^ a b c d Zschaechner, Laura K.; Rand, Richard J.; Walterbos, Rene (2015-01-15). "Investigating Disk-Halo Flows and Accretion: A Kinematic and Morphological Analysis of Extraplanar H I in NGC 3044 and NGC 4302". The Astrophysical Journal. 799 (1): 61. arXiv:1411.2593. Bibcode:2015ApJ...799...61Z. doi:10.1088/0004-637X/799/1/61. ISSN 1538-4357. S2CID 119118897.
- ^ a b c d e Vlahakis, C.; Verstappen, J.; Smith, M. W. L.; Pohlen, M.; Grossi, M.; Fritz, J.; Looze, I. De; Clemens, M.; Ciesla, L. (2012-09-01). "The Herschel Virgo Cluster Survey - XI. Environmental effects on molecular gas and dust in spiral disks". Astronomy & Astrophysics. 545: A75. arXiv:1207.5051. Bibcode:2012A&A...545A..75P. doi:10.1051/0004-6361/201219689. ISSN 0004-6361. S2CID 53701670.
- ^ a b c d Chemin, L.; Balkowski, C.; Cayatte, V.; Carignan, C.; Amram, P.; Garrido, O.; Hernandez, O.; Marcelin, M.; Adami, C. (2006-03-01). "A Virgo high-resolution Halpha kinematical survey - II. The Atlas". Monthly Notices of the Royal Astronomical Society. 366 (3): 812–857. arXiv:astro-ph/0511417. Bibcode:2006MNRAS.366..812C. doi:10.1111/j.1365-2966.2005.09899.x. ISSN 0035-8711. S2CID 16780630.
- ^ Elmegreen, Debra Meloy; Chromey, Frederick R.; Bissell, Bradley A.; Corrado, Kelli (1999-12-01). "K'-Band Observations of Underlying Symmetric Structure in Flocculent Galaxies". The Astronomical Journal. 118 (6): 2618–2624. Bibcode:1999AJ....118.2618E. doi:10.1086/301127. ISSN 0004-6256.
- ^ Elmegreen, D. M. (1981-11-01). "A near-infrared atlas of spiral galaxies". The Astrophysical Journal Supplement Series. 47: 229–233. Bibcode:1981ApJS...47..229E. doi:10.1086/190757. ISSN 0067-0049.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-03-10.
- ^ "New General Catalog Objects: NGC 4250 - 4299". cseligman.com. Retrieved 2018-08-14.
- ^ Binggeli, B.; Sandage, A.; Tammann, G. A. (September 1985). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area. V - Luminosity functions of Virgo Cluster galaxies". The Astronomical Journal. 90: 1681. Bibcode:1985AJ.....90.1681B. doi:10.1086/113874. ISSN 0004-6256.
- ^ R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN 978-0-521-35299-4.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-03-10.
- ^ Davis, Benjamin L.; Soria, Roberto; Graham, Alister W. (2019). "Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies". Monthly Notices of the Royal Astronomical Society. 484 (1): 814. arXiv:1811.03232. Bibcode:2019MNRAS.484..814G. doi:10.1093/mnras/sty3068. S2CID 119303249.
- ^ a b c Vollmer, B.; Soida, M.; Beck, R.; Chung, A.; Urbanik, M.; Chyży, K. T.; Otmianowska-Mazur, K.; Kenney, J. D. P. (May 2013). "Large-scale radio continuum properties of 19 Virgo cluster galaxies: The influence of tidal interactions, ram pressure stripping, and accreting gas envelopes". Astronomy & Astrophysics. 553: A116. arXiv:1304.1279. Bibcode:2013A&A...553A.116V. doi:10.1051/0004-6361/201321163. ISSN 0004-6361. S2CID 119190841.
- ^ a b Weżgowiec, M.; Urbanik, M.; Beck, R.; Chyży, K. T.; Soida, M. (September 2012). "The magnetic fields of large Virgo cluster spirals. II". Astronomy & Astrophysics. 545: A69. arXiv:1208.2845. Bibcode:2012A&A...545A..69W. doi:10.1051/0004-6361/201218871. ISSN 0004-6361. S2CID 6957500.
- ^ a b c d Chung, Aeree; van Gorkom, J. H.; Kenney, Jeffrey D. P.; Crowl, Hugh; Vollmer, Bernd (2009-12-01). "Vla Imaging of Virgo Spirals in Atomic Gas (Viva). I. The Atlas and the H I Properties". The Astronomical Journal. 138 (6): 1741–1816. Bibcode:2009AJ....138.1741C. doi:10.1088/0004-6256/138/6/1741. ISSN 0004-6256.
- ^ a b Chung, E. J.; Rhee, M.-H.; Kim, H.; Yun, Min S.; Heyer, M.; Young, J. S. (2009-10-01). "12 Co( J = 1 – 0) On-The-Fly Mapping Survey of the Virgo Cluster Spirals. I. Data and Atlas". The Astrophysical Journal Supplement Series. 184 (2): 199–217. arXiv:0910.3465. Bibcode:2009ApJS..184..199C. doi:10.1088/0067-0049/184/2/199. ISSN 0067-0049. S2CID 118808228.
- ^ a b Saha, Kanak; de Jong, Roelof; Holwerda, Benne (2009-06-11). "The onset of warps in Spitzer observations of edge-on spiral galaxies". Monthly Notices of the Royal Astronomical Society. 396 (1): 409–422. arXiv:0902.4436. Bibcode:2009MNRAS.396..409S. doi:10.1111/j.1365-2966.2009.14696.x. S2CID 16352978.
- ^ a b Hota, Ananda. "GMRT Observations of the Group Holmberg 124". Ncra.tifr.res.in.
- ^ Malin, D. (1994). "Interacting Galaxies in the Virgo Cluster". Astronomy from Wide-Field Imaging. 161: 567–576. Bibcode:1994IAUS..161..567M. doi:10.1007/978-94-011-1146-1_119. ISBN 978-0-7923-2879-7. S2CID 118943109.
- ^ Chung, Aeree; van Gorkom, J. H.; Kenney, Jeffrey D. P.; Vollmer, Bernd (2007-04-01). "Virgo Galaxies with Long One-sided H I Tails". The Astrophysical Journal Letters. 659 (2): L115–L119. arXiv:astro-ph/0703338. Bibcode:2007ApJ...659L.115C. doi:10.1086/518034. ISSN 0004-637X. S2CID 13021118.
External links
Wikimedia Commons has media related to NGC 4298.
- NGC 4298 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
This page was last edited on 12 August 2023, at 16:48