NGC 705

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NGC 705
NGC 705 PanS.jpg
Pan-STARRS image of NGC 705
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 01h 52m 41.5s [1]
Declination 36° 08′ 38″ [1]
Redshift 0.015057 [1]
Helio radial velocity 4514 km/s [1]
Distance 190  Mly (58.2  Mpc) [1]
Group or cluster Abell 262
Apparent magnitude  (V)14.63 [1]
Characteristics
Type S0/a [1]
Size~69,000  ly (21.2  kpc) (estimated) [1]
Apparent size  (V)1.2 x 0.3 [1]
Other designations
6ZW 90, CGCG 522-36, MCG 6-5-30, PGC 6958, UGC 1345 [1]

NGC 705 is a lenticular galaxy located 240 million light-years away [2] in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 [3] and is also a member of Abell 262. [4] [5] [6] [7]

Contents

Although NGC 705 is an early type galaxy, it has a dust lane that is concentrated toward its central region. It is projected to lie about 0.098  Mly (0.03  Mpc ) from the cd-galaxy NGC 708. [7]

See also

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<span class="mw-page-title-main">NGC 708</span> Galaxy in the constellation Andromeda

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

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

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<span class="mw-page-title-main">NGC 4093</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4324</span> 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 705. Retrieved 2018-11-23.
  2. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-11-24.
  3. ↑ "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2018-11-21.
  4. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-11-24.
  5. ↑ 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.
  6. ↑ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178. arXiv: astro-ph/0001140 . Bibcode:2000ApJ...543..178G. doi:10.1086/317070. ISSN   0004-637X. S2CID   9618325.
  7. 1 2 Santiago, B. X.; Vale, T. B. (2008-05-06). "Deep surface photometry of edge-on spirals in Abell galaxy clusters". Astronomy & Astrophysics. 485 (1): 21–31. arXiv: 0804.4653 . doi:10.1051/0004-6361:20079281. ISSN   0004-6361. S2CID   15104510.


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