MCG+04-05-011, VV 338, 2MASX J01475452+2725580, IRAS 01450+2710, NGC 672, UGC 1256, PGC 6595[9]
NGC 672 is a spiral galaxy in the northern constellation of Triangulum, positioned around 2° to the southwest of the star Alpha Trianguli.[10] The original object designated NGC 672 was discovered by the German-born astronomer William Herschel on 26 October 1786, but this was later cataloged as NGC 614. The object now identified as NGC 672 was discovered by John Herschel on 11 November 1827.[11]This link refers to NGC 627, not NGC 672
This galaxy is located at a distance of approximately 23.4 megalight-years from the Milky Way,[4] where it forms an interacting pair with the irregular galaxy IC 1727.[12][13] In the neutral hydrogen radio band, a tidal bridge is observed between the galaxies.[14] NGC 672 appears to be the more massive of the two, and hence IC 1727 shows more distortion from the interaction.[7] Together they form members of a combined group of galaxies that includes NGC 784.[15]
The morphological classification of NGC 672 is SB(s)cd,[6] which indicates this is a barred spiral galaxy (SB), with no ring structure around the central bar (s), and moderately to loosely-wound spiral arms. In the visual spectrum, the galaxy appears symmetrical with clearly defined spiral arms.[14] It is gas-rich with an estimated mass of 38 billion times the mass of the Sun and a star formation rate of 0.3 M☉ yr−1.[7]
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NGC672 is a spiral galaxy in the northern constellation of Triangulum, positioned around 2° to the southwest of the star Alpha Trianguli. The original...
include the 10 arcminute long magnitude 12 NGC 925 spiral galaxy and the 5 arcminute long magnitude 11.6 NGC672 barred spiral galaxy. The latter is close...
00/2008 Bibcode:2008ralc.conf..358W Zitrin, A.; Brosch, N. (2008). "The NGC672 and 784 galaxy groups: evidence for galaxy formation and growth along a...
Possible members: NGC672, IC 1727, NGC 1156(?). Possible (dwarfs): DDO 011, DDO 017, DDO 019, DDO 022, DDO 026. The location of the NGC 1023 group within...
Inflowing Molecular Gas in NGC 1275 Deposited by an X-Ray Cooling Flow in the Perseus Cluster". The Astrophysical Journal. 672 (1): 252–265. arXiv:0712...
Extragalactic Database". Results for NGC 784. Retrieved 17 February 2013. Zitrin, Adi; Brosch, Noah (26 July 2008). "The NGC672 and 784 galaxy groups: evidence...
composite pseudo-bulge galaxies NGC 3368 and NGC 3489". Monthly Notices of the Royal Astronomical Society. 403 (2): 646–672. arXiv:0912.2511. Bibcode:2010MNRAS...
difficult to observe. "PGC 39058". NASA/IPAC Extragalactic Database. "NGC672". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 December...
The NGC 5866 Group is a small group of galaxies located in the constellation Draco. The group is named after NGC 5866, the galaxy with the highest apparent...
composite pseudo-bulge galaxies NGC 3368 and NGC 3489", Monthly Notices of the Royal Astronomical Society, 403 (2): 646–672, arXiv:0912.2511, Bibcode:2010MNRAS...
2005). "Infall of the Elliptical Galaxy NGC 1404 into the Fornax Cluster". The Astrophysical Journal. 621 (2): 663–672. arXiv:astro-ph/0408159. Bibcode:2005ApJ...
galaxy NGC 4789A NGC 4565 (Needle Galaxy) NGC 4651, with umbrella-shaped stellar streams The constellation Coma Berenices hosts the galaxy NGC 4495 among...
composite pseudo-bulge galaxies NGC 3368 and NGC 3489". Monthly Notices of the Royal Astronomical Society. 403 (2): 646–672. arXiv:0912.2511. Bibcode:2010MNRAS...
Milky Way itself. NGC 3172 (also known as Polarissima Borealis) is a faint, magnitude-14.9 galaxy that happens to be the closest NGC object to the north...
NGC 613 is a barred spiral galaxy located 67 million light years away in the southern constellation of Sculptor. This galaxy was discovered in 1798 by...
massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region". Astronomy & Astrophysics. 456 (2): 623–638...
Kris; Grammer, Skyler H. (January 2019). "Luminous and Variable Stars in NGC 2403 and M81". The Astronomical Journal. 157 (1): 22. arXiv:1811.06559. Bibcode:2019AJ...
instruments sensitive to the far infrared and submillimetre wavebands (55–672 μm). Herschel was the fourth and final cornerstone mission in the Horizon...