NGC 4319
NGC 4319 | |
---|---|
观测资料(J2000 曆元) | |
星座 | 天龍座 |
赤经 | 12h 21m 43.846s[1] |
赤纬 | +75° 19′ 21.45″[1] |
紅移 | 0.004526[2] |
徑向速度 | 1,357 ± 46[3] km/s |
距离 | 76.6 Mly (23.48 Mpc)[3] |
视星等 (V) | 12.8[2] |
特征 | |
类型 | SB(r)ab[4] |
角直徑 (V) | 3′.0 × 2′.3[2] |
其他名称 | |
NGC 4345, UGC 7429,[2] PGC 39981[2] | |
NGC 4319是一個棒旋星系,位於天龍座,距離地球約7,700萬光年。形態分類為SB(r)ab,顯示它是一種具有內環結構和中度至緊密纏繞臂的棒狀螺旋[5]。NGC 4319位置靠近NGC 4291和NGC 4386星系,中間間隙發出的X射線顯示NGC 4319與NGC 4291可能正在相互作用。與銀河系相比,NGC 4319的電離氫比例要高得多[6]。
1971年,美國天文學家赫頓·阿普注意到NGC 4319和馬卡萊恩205之間似乎存在物理聯繫,馬卡萊恩205是一顆具有更高紅移的類星體。他認為,如果馬卡萊恩205不是背景天體,那麼它可能是從這個星系的核心噴射出來的[7]。兩者之間明顯發光聯繫引起一場天文學家之間的爭議,其他天文學家試圖反駁這一說法並提供解釋[8]。哈伯太空望遠鏡的觀測表明,來自馬卡萊恩205的光線穿過NGC 4319 的圓盤和光暈到達地球,顯示馬卡萊恩205其實是一個背景天體[9]。
參考資料
- ^ 1.0 1.1 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. The Two Micron All Sky Survey (2MASS). The Astronomical Journal. 1 February 2006, 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. ISSN 0004-6256. S2CID 18913331. doi:10.1086/498708 .
- ^ 2.0 2.1 2.2 2.3 2.4 NASA/IPAC Extragalactic Database. Results for NGC 4319. [2007-03-30].
- ^ 3.0 3.1 Crook, Aidan C.; et al, Groups of Galaxies in the Two Micron All Sky Redshift Survey, The Astrophysical Journal, February 2007, 655 (2): 790–813, Bibcode:2007ApJ...655..790C, S2CID 11672751, arXiv:astro-ph/0610732 , doi:10.1086/510201.
- ^ Erwin, Peter; Debattista, Victor P., Peanuts at an angle: detecting and measuring the three-dimensional structure of bars in moderately inclined galaxies, Monthly Notices of the Royal Astronomical Society, June 2013, 431 (4): 3060–3086, Bibcode:2013MNRAS.431.3060E, S2CID 54653263, arXiv:1301.0638 , doi:10.1093/mnras/stt385 .
- ^ Buta, Ronald J.; et al, Atlas of Galaxies, Cambridge University Press: 13–17, 2007, ISBN 978-0521820486.
- ^ Bowen, David V.; Blades, J. C., Interstellar MG II and C IV absorption toward Markarian 205 by NGC 4319 - an 'optically thick' QSO absorption system, Astrophysical Journal Letters, February 1993, 403 (2): L55–L58, 646, Bibcode:1993ApJ...403L..55B, doi:10.1086/186720.
- ^ Arp, H., A Connection Between the Spiral Galaxy NGC 4319 and the Quasi-Stellar Object Markarian 205, Astrophysical Letters, August 1971, 9: 1, Bibcode:1971ApL.....9....1A.
- ^ Sulentic, J. W., Confirmation of the luminous connection between NGC 4319 and Markarian 205, Astrophysical Journal Letters, February 1983, 265: L49–L53, Bibcode:1983ApJ...265L..49S, doi:10.1086/183956 .
- ^ Bahcall, John N.; et al, The near-ultraviolet spectrum of Markarian 205, Astrophysical Journal, Part 1, October 1992, 398 (2): 495–500, 646, Bibcode:1992ApJ...398..495B, doi:10.1086/171872.
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