NGC 679

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NGC 679
2MASS NGC 679.jpg
2MASS image of NGC 679.
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 01h 49m 43.8s [1]
Declination 35° 47′ 08″ [1]
Redshift 0.016842 [1]
Helio radial velocity 5049 km/s [1]
Distance 213  Mly (65.4  Mpc) [1]
Group or cluster Abell 262
Apparent magnitude  (V)13.33 [1]
Characteristics
Type E, [2] S0^- [1]
Size~106,000  ly (32.4  kpc) (estimated) [1]
Apparent size  (V)2.1 x 2.1 [1]
Other designations
CGCG 522-15, MCG 6-5-12, PGC 6711, UGC 1283 [1]

NGC 679 is an elliptical [3] [4] [5] or a lenticular galaxy [6] [4] [5] located 210 million light-years away [6] in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 13, 1784 [7] and is a member of Abell 262. [8] [9] [10] [11] [12]

Contents

It is also a radio galaxy. [13]

Dust Disk

NGC 679 hosts a nearly face-on disk of dust with a diameter of ~9,800  ly (3  kpc ). [3]

NGC 679 (DSS) NGC 0679 DSS.jpg
NGC 679 (DSS)

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 669</span> Galaxy in the constellation Triangulum

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<span class="mw-page-title-main">NGC 687</span> Lenticular galaxy in constellation Andromeda

NGC 687 is a lenticular galaxy located 220 million light-years away in the constellation Andromeda. It was discovered by astronomer William Herschel on September 21, 1786 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 688</span> Barred spiral galaxy in the constellation Triangulum

NGC 688 is a barred spiral galaxy with starburst activity located 190 million light-years away in the constellation Triangulum. It was discovered by astronomer Heinrich d'Arrest on September 16, 1865 and is a member of the galaxy cluster Abell 262.

<span class="mw-page-title-main">NGC 700</span> Lenticular galaxy in constellation Andromeda

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<span class="mw-page-title-main">NGC 703</span> Lenticular galaxy in the constellation Andromeda

NGC 703 is a lenticular galaxy located 240 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.

<span class="mw-page-title-main">NGC 704</span> Lenticular galaxy in the constellation Andromeda

NGC 704 is a lenticular galaxy located 220 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.

<span class="mw-page-title-main">NGC 705</span> Lenticular galaxy in the constellation Andromeda

NGC 705 is a lenticular galaxy located 240 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.

<span class="mw-page-title-main">NGC 709</span> Lenticular galaxy in the constellation Andromeda

NGC 709 is a lenticular galaxy located 150 million light-years away in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 and is a member of the galaxy cluster Abell 262.

<span class="mw-page-title-main">NGC 712</span> Lenticular galaxy in constellation Andromeda

NGC 712 is a lenticular galaxy located 230 million light-years away in the constellation Andromeda. It was discovered by astronomer John Herschel in October 1828 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 714</span> Lenticular galaxy in constellation Andromeda

NGC 714 is a lenticular galaxy located 190 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer Bindon Blood Stoney on October 28, 1850 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 717</span> Lenticular galaxy in constellation Andromeda

NGC 717 is a lenticular galaxy located 210 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer Bindon Blood Stoney on October 28, 1850 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 753</span> Spiral galaxy in the constellation Andromeda

NGC 753 is a spiral galaxy located 220 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer by Heinrich d'Arrest on September 16, 1865 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 759</span> Elliptical galaxy in the constellation Andromeda

NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865. It is a member of Abell 262.

<span class="mw-page-title-main">NGC 4513</span> Lenticular galaxy in the constellation Draco

NGC 4513 is a lenticular galaxy and a ring galaxy located about 110 million light-years away in the constellation Draco. It was discovered by astronomer Heinrich d'Arrest on October 16, 1866.

<span class="mw-page-title-main">NGC 3937</span> Elliptical or lenticular galaxy in the constellation Leo

NGC 3937 is an elliptical or a lenticular galaxy located about 310 million light-years away in the constellation Leo. It was discovered by astronomer William Herschel on April 27, 1785 and is classified as a radio galaxy.

<span class="mw-page-title-main">NGC 4324</span> Lenticular galaxy in the constellation of Virgo

NGC 4324 is a lenticular galaxy located about 85 million light-years away in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on March 4, 1862. NGC 4324 has a stellar mass of 5.62 × 1010M☉, and a baryonic mass of 5.88 × 1010M☉. The galaxy's total mass is around 5.25 × 1011M☉. NGC 4324 is notable for having a ring of star formation surrounding its nucleus. It was considered a member of the Virgo II Groups until 1999, when its distance was recalculated and it was placed in the Virgo W Group.

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 679. Retrieved 2018-11-16.
  2. ↑ "HyperLeda Database". Results for NGC 679. Retrieved 2018-11-16.
  3. 1 2 Wegner, G. A.; Corsini, E. M.; Thomas, J.; Saglia, R. P.; Bender, R.; Pu, S. B. (2012). "Further Evidence for Large Central Mass-to-light Ratios in Early-type Galaxies: The Case of Ellipticals and Lenticulars in the A262 Cluster". The Astronomical Journal. 144 (3): 78. arXiv: 1206.5768 . Bibcode:2012AJ....144...78W. doi:10.1088/0004-6256/144/3/78. ISSN   1538-3881. S2CID   118679035.
  4. 1 2 "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved 2018-11-17.
  5. 1 2 "NGC 0679" . Retrieved 2018-11-17.
  6. 1 2 "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-11-17.
  7. ↑ "New General Catalog Objects: NGC 650 - 699". cseligman.com. Retrieved 2018-11-14.
  8. ↑ P., Fouque; E., Gourgoulhon; P., Chamaraux; G., Paturel (May 1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement Series. 93: 211. Bibcode:1992A&AS...93..211F. ISSN   0365-0138.
  9. ↑ M., Garcia, A. (July 1993). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G. ISSN   0365-0138.
  10. ↑ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (November 2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178–194. arXiv: astro-ph/0001140 . Bibcode:2000ApJ...543..178G. doi:10.1086/317070. ISSN   0004-637X. S2CID   9618325.
  11. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-11-17.
  12. ↑ "NGC 679" . Retrieved 2018-11-20.
  13. ↑ G., Righetti; G., Giovannini; L., Feretti (April 1988). "WSRT observations at 327 MHz of the cluster A262". Astronomy and Astrophysics Supplement Series. 73: 173. Bibcode:1988A&AS...73..173R. ISSN   0365-0138.
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