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NGC 672 information


NGC 672
NGC 672, imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationTriangulum
Right ascension01h 47m 54.47627s[1]
Declination+27° 25′ 57.9948″[1]
Redshift0.001403[2]
Heliocentric radial velocity425[3] km/s
Distance23.42 ± 0.33 Mly (7.18 ± 0.10 Mpc)[4]
Apparent magnitude (V)11.09±0.03[5]
Characteristics
TypeSB(s)cd[6]
Mass3.8×1010 M[7] M
Apparent size (V)6′.17 × 2′.29[8]
Other designations
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]

  1. ^ a b Cite error: The named reference GaiaDR2 was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference Kochanek2001 was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference tully2016 was invoked but never defined (see the help page).
  4. ^ a b Cite error: The named reference Tully2013 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference Cook2014 was invoked but never defined (see the help page).
  6. ^ a b Cite error: The named reference Konstantopoulos2013 was invoked but never defined (see the help page).
  7. ^ a b c Cite error: The named reference Ramirez-Ballinas2014 was invoked but never defined (see the help page).
  8. ^ Cite error: The named reference Paturel2003 was invoked but never defined (see the help page).
  9. ^ Cite error: The named reference simbad was invoked but never defined (see the help page).
  10. ^ Cite error: The named reference Sinnott1997 was invoked but never defined (see the help page).
  11. ^ Cite error: The named reference cseligman was invoked but never defined (see the help page).
  12. ^ Cite error: The named reference Tikhonov2014 was invoked but never defined (see the help page).
  13. ^ Cite error: The named reference Combes1980 was invoked but never defined (see the help page).
  14. ^ a b Cite error: The named reference Stanchfield2012 was invoked but never defined (see the help page).
  15. ^ Cite error: The named reference McQuinn2014 was invoked but never defined (see the help page).

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NGC 672

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NGC 672 is a spiral galaxy in the northern constellation of Triangulum, positioned around 2° to the southwest of the star Alpha Trianguli. The original...

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include the 10 arcminute long magnitude 12 NGC 925 spiral galaxy and the 5 arcminute long magnitude 11.6 NGC 672 barred spiral galaxy. The latter is close...

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NGC 784

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NGC 3489

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Herschel Space Observatory

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