NGC 709

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NGC 709
NGC 709 PanS.jpg
Pan-STARRS image of NGC 709
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 01h 52m 50.6s [1]
Declination 36° 13′ 24″ [1]
Redshift 0.011928 [1]
Helio radial velocity 3576 km/s [1]
Distance 150  Mly (45  Mpc) [1]
Group or cluster Abell 262
Apparent magnitude  (V)15.23 [1]
Characteristics
Type S0 [1]
Size~46,000  ly (14  kpc) (estimated) [1]
Apparent size  (V)0.6 x 0.3 [1]
Other designations
PGC 006969 [1]

NGC 709 is a lenticular galaxy located 150 million light-years away [2] in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 [3] and is a member of the galaxy cluster Abell 262. [4] [5] [6] [7] [8] [9]

Contents

See also

Related Research Articles

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NGC 4709 is an elliptical galaxy located in the constellation Centaurus. It is considered to be a member of the Centaurus Cluster and is the dominant member of a small group of galaxies known as "Cen 45" which is currently merging with the main Centaurus Cluster even though the two subclusters' line of sight redshift velocities differ by about 1500 km/s. NGC 4709 was discovered by astronomer James Dunlop on May 7, 1826.

<span class="mw-page-title-main">NGC 1272</span> Galaxy in the constellation Perseus

NGC 1272 is a massive elliptical galaxy located about 230 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1272 has an active nucleus and is the second brightest member of the Perseus Cluster after NGC 1275.

<span class="mw-page-title-main">NGC 1278</span> Galaxy in the constellation Perseus

NGC 1278 is an elliptical galaxy located about 230 million light-years away in the constellation Perseus. NGC 1278 was discovered by astronomer Heinrich d'Arrest on February 14, 1863. It was then rediscovered by astronomer Guillaume Bigourdan on October 22, 1884 and was later listed as IC 1907. NGC 1278 is a member of the Perseus Cluster and is a low-luminosity AGN (LLAGN).

<span class="mw-page-title-main">NGC 1281</span> Galaxy in the constellation Perseus

NGC 1281 is a compact elliptical galaxy located about 200 million light-years away in the constellation Perseus. NGC 1281 was discovered by astronomer John Dreyer on December 12, 1876. It is a member of the Perseus Cluster.

<span class="mw-page-title-main">NGC 1283</span> Galaxy in the constellation Perseus

NGC 1283 is an elliptical galaxy located about 250 million light-years away in the constellation Perseus. The galaxy was discovered by astronomer Guillaume Bigourdan on October 23, 1884 and is a member of the Perseus Cluster. It also contains an active galactic nucleus.

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

NGC 708 is an elliptical galaxy located 240 million light-years away in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786. It is classified as a cD galaxy and is the brightest member of Abell 262. NGC 708 is a weak FR I radio galaxy and is also classified as a type 2 Seyfert galaxy.

<span class="mw-page-title-main">NGC 668</span> Galaxy in constellation Andromeda

NGC 668 is a spiral galaxy located 200 million light-years away in the constellation Andromeda. It was discovered by astronomer Édouard Stephan on December 4, 1880 and is a member of Abell 262.

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

NGC 669 is an edge-on spiral galaxy with an active galactic nucleus located 200 million light-years away in the constellation Triangulum. NGC 669 was discovered by astronomer Édouard Stephan on November 28, 1883 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 679</span> Galaxy in the constellation Andromeda

NGC 679 is an elliptical or a lenticular galaxy located 210 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 13, 1784 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 687</span> 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> 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 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

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> 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 710</span> Galaxy in the constellation Andromeda

NGC 710 is a spiral galaxy located 260 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> 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> 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> 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> 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> 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.

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 709. Retrieved 2018-12-26.
  2. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-12-27.
  3. ↑ "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2018-11-21.
  4. ↑ "NGC 709". sim-id. Retrieved 2018-12-27.
  5. ↑ Steinicke, Wolfgang (2010-08-19). Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press. p. 309. ISBN   978-1-139-49010-8.
  6. ↑ Scodeggio, Marco; Boselli, Alessandro; Gavazzi, Giuseppe; Trinchieri, Ginevra; Garilli, Bianca (1992-08-01). "Multifrequency windows on spiral galaxies. II - The A262 and Cancer clusters". Astronomy and Astrophysics Supplement Series. 94: 299–326. Bibcode:1992A&AS...94..299S. ISSN   0365-0138.
  7. ↑ Butcher, H. R.; Oemler, A. Jr. (1985-04-01). "The evolution of galaxies in clusters. IV - Photometry of 10 low-redshift clusters". The Astrophysical Journal Supplement Series. 57: 665–691. Bibcode:1985ApJS...57..665B. doi:10.1086/191022. ISSN   0067-0049.
  8. ↑ Fanti, C.; Fanti, R.; Feretti, L.; Ficarra, A.; Gioia, I. M.; Giovannini, G.; Gregorini, L.; Mantovani, F.; Marano, B. (1982-01-01). "Radio and optical observations of 9 nearby Abell clusters - A262, A347, A569, A576, A779, A1213, A1228, A2162, A2666". Astronomy and Astrophysics. 105: 200–218. Bibcode:1982A&A...105..200F. ISSN   0004-6361.
  9. ↑ Moss, C.; Dickens, R. J. (1977-03-01). "Redshifts of galaxies in the cluster Abell 262, and in the region of the Pisces group /centred on NGC 383/". Monthly Notices of the Royal Astronomical Society. 178 (4): 701–715. Bibcode:1977MNRAS.178..701M. doi: 10.1093/mnras/178.4.701 . ISSN   0035-8711.


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