NGC 7001

Last updated
NGC 7001
NGC7001 - SDSS DR14.jpg
The intermediate spiral galaxy NGC 7001 (SDSS DR14)
Observation data (J2000 epoch)
Constellation Aquarius
Right ascension 21h 01m 07.7s [1]
Declination −00° 11′ 43″ [1]
Redshift 0.023714 [1]
Heliocentric radial velocity 7109 [1] km/s
Distance 302  Mly (92.7  Mpc) [1]
Apparent magnitude  (V)13.8 [1]
Characteristics
Type SAB(rs)ab [1]
Mass 4.8×1011 (Stellar mass) [2]   M☉
Size~123,100  ly (37.74  kpc) (estimated) [1]
Apparent size  (V)1.25 × 1.06 [1]
Other designations
NPM1G -00.0540, IRAS 20585-0023, UGC 11663, MCG +00-53-016, PGC 65905, CGCG 374-37 [1]

NGC 7001 is an intermediate spiral galaxy [3] located about 300 million light-years away [3] in the constellation Aquarius. [4] NGC 7001 has an estimated diameter of 123,000 light-years. [3] It was discovered by English astronomer John Herschel on July 21, 1827, and was also observed by Austrian astronomer Rudolf Spitaler on September 26, 1891. [5]

Contents

NGC 7001 has tightly wound spiral arms similar to the galaxy NGC 488. [6] The galaxy is also host to a supermassive black hole with an estimated mass of 7 × 107 M☉. [7]

See also

Related Research Articles

<span class="mw-page-title-main">NGC 7002</span> Galaxy in the constellation Indus

NGC 7002 is a large elliptical galaxy, and a radio galaxy, around 320 million light-years away from Earth in the constellation of Indus. The galaxy was discovered by English astronomer John Herschel on September 30, 1834. NGC 7002 is the brightest member of a group of galaxies known as [T2015] nest 200093. The group contains 12 member galaxies including NGC 7004, has a velocity dispersion of 440 km/s and an estimated mass of 1.28 × 1014M☉. NGC 7002 is also host to a supermassive black hole with an estimated mass of 2.7 × 109M☉.

<span class="mw-page-title-main">NGC 7003</span> Galaxy in the constellation Delphinus

NGC 7003 is a spiral galaxy around 220 million light-years from Earth in the constellation Delphinus. NGC 7003 has an estimated diameter of 85,000 light-years. The galaxy was discovered by German astronomer Heinrich Louis d'Arrest on August 26, 1864.

<span class="mw-page-title-main">NGC 7004</span> Spiral galaxy in the constellation Indus

NGC 7004 is a lenticular galaxy and a type 2 Seyfert galaxy around 330 million light-years away from Earth in the constellation Indus. NGC 7004 has an estimated diameter of 140,000 light-years. NGC 7004 was discovered by astronomer John Herschel on October 2, 1834. NGC 7004 is a member of a group of galaxies known as [T2015] nest 200093. The group contains 12 member galaxies including NGC 7002, has a velocity dispersion of 440 km/s and an estimated mass of 1.28 × 1014M☉. NGC 7004 is also host to a supermassive black hole with an estimated mass of 8.1 × 108M☉.

<span class="mw-page-title-main">NGC 7007</span> Galaxy in the constellation Indus

NGC 7007 is a lenticular galaxy with a small bar, around 100 million light-years away from Earth in the constellation Indus. It was discovered by astronomer John Herschel on July 8, 1834. The galaxy is a type 2 seyfert galaxy, and is host to a supermassive black hole with an estimated mass of 4.9 × 107M☉.

<span class="mw-page-title-main">NGC 7010</span> Galaxy in the constellation Aquarius

NGC 7010 is a massive elliptical galaxy located about 370 million light-years from Earth in the constellation Aquarius. NGC 7010 was discovered by astronomer John Herschel on August 6, 1823, and was later listed by French astronomer Guillaume Bigourdan as IC 5082. It is host to a supermassive black hole with an estimated mass of 4.7 × 108M☉.

<span class="mw-page-title-main">NGC 7015</span> Spiral galaxy in the constellation Equuleus

NGC 7015 is a spiral galaxy located about 203 million light-years away from Earth in the constellation Equuleus. NGC 7015's calculated velocity is 4,881 km/s (3,033 mi/s). NGC 7015 was discovered by French astronomer Édouard Stephan on September 29, 1878.

<span class="mw-page-title-main">NGC 7019</span> Galaxy in the constellation Capricornus

NGC 7019 is a spiral galaxy located about 480 million light-years away in the constellation of Capricornus. It was discovered by American astronomer Francis Leavenworth in 1886. It is host to a supermassive black hole with an estimated mass of with an estimated mass of 7.5 × 107M☉.

<span class="mw-page-title-main">NGC 1436</span> Galaxy in the constellation Eridanus

NGC 1436 is a barred spiral galaxy with LINER activity approximately 58 million light-years away from Earth in the constellation of Eridanus. NGC 1436 is a flocculent spiral galaxy lying almost face-on to the Earth. It is a member of the Fornax I cluster.

<span class="mw-page-title-main">NGC 4596</span> Galaxy in the constellation Virgo

NGC 4596 is a barred lenticular galaxy located about 55 million light-years away in the constellation Virgo. NGC 4596 was discovered by astronomer William Herschel on March 15, 1784. NGC 4596 is a member of the Virgo Cluster and has an inclination of about 38°.

<span class="mw-page-title-main">NGC 4709</span> Galaxy in the constellation Centaurus

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 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 3860</span> Spiral galaxy in the constellation Leo

NGC 3860 is a spiral galaxy located about 340 million light-years away in the constellation Leo. NGC 3860 was discovered by astronomer William Herschel on April 27, 1785. The galaxy is a member of the Leo Cluster and is a low-luminosity AGN (LLAGN). Gavazzi et al. however classified NGC 3860 as a strong AGN which may have been triggered by a supermassive black hole in the center of the galaxy.

<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 4299</span> Spiral galaxy in the constellation Virgo

NGC 4299 is a featureless spiral galaxy located about 55 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4313</span> Spiral galaxy in the constellation Virgo

NGC 4313 is an edge-on spiral galaxy located about 50 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784. NGC 4313 is a member of the Virgo Cluster and is classified as LINER and as a Seyfert galaxy.

<span class="mw-page-title-main">NGC 1369</span> Galaxy of the Fornax Cluster

NGC 1369 is a barred lenticular galaxy located 59 millon light years away in constellation of Eridanus. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster. NGC 1369 is a host to a supermassive black hole with an estimated mass of 1.8 millon solar masses.

<span class="mw-page-title-main">NGC 1428</span> Galaxy in the constellation Fornax

NGC 1428 is a peculiar galaxy of an uncertain morphology; either an elliptical or lenticular galaxy located approximately 65 million light-years away from Earth.

<span class="mw-page-title-main">NGC 4393</span> Galaxy in the constellation of Coma Berenices

NGC 4393 is a spiral galaxy about 46 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 11, 1785. It is a member of the NGC 4274 Group, which is part of the Coma I Group or Cloud.

<span class="mw-page-title-main">NGC 4328</span> Galaxy in the constellation Coma Berenices

NGC 4328 is a nucleated dwarf elliptical or lenticular galaxy located about 48 million light-years away based on observations by the Hubble Space Telescope using the TRGB distance indicator. NGC 4328 was discovered on March 21, 1784 by astronomer William Herschel and is a member of the Virgo Cluster in the "A'' subgroup. On the sky, NGC 4328 is located in the constellation Coma Berenices.

<span class="mw-page-title-main">NGC 4310</span> Dwarf spiral galaxy in the constellation Coma Berenices

NGC 4310 is a dwarf spiral galaxy with a dust lane and ring structure located about 54 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 11, 1785. It was rediscovered by astronomer Heinrich d'Arrest on May 19, 1863, and was later listed as NGC 4338. The galaxy is host to a supermassive black hole with an estimated mass of 107 solar masses.

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 7001. Retrieved 2017-04-13.
  2. ↑ Wilman, David J.; Fontanot, Fabio; De Lucia, Gabriella; Erwin, Peter; Monaco, Pierluigi (2013-08-01). "The hierarchical origins of observed galaxy morphology". Monthly Notices of the Royal Astronomical Society. 433 (4): 2986–3004. arXiv: 1305.7163 . Bibcode:2013MNRAS.433.2986W. doi: 10.1093/mnras/stt941 . ISSN   0035-8711.
  3. 1 2 3 "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-04-15.
  4. ↑ Rojas, Sebastián García. "Galaxy NGC 7001 · Deep Sky Objects Browser". DSO Browser. Archived from the original on 2017-05-24. Retrieved 2017-04-15.
  5. ↑ "New General Catalog Objects: NGC 7000 – 7049". cseligman.com. Retrieved 2017-04-15.
  6. ↑ Buta, Ronald J. (2019-09-01). "The systematics of galaxy morphology in the comprehensive de Vaucouleurs revised Hubble-Sandage classification system: application to the EFIGI sample". Monthly Notices of the Royal Astronomical Society. 488 (1): 590–608. arXiv: 1906.08124 . Bibcode:2019MNRAS.488..590B. doi: 10.1093/mnras/stz1693 . ISSN   0035-8711.
  7. ↑ Arzoumanian, Zaven; Baker, Paul T.; Brazier, Adam; Brook, Paul R.; Burke-Spolaor, Sarah; Becsy, Bence; Charisi, Maria; Chatterjee, Shami; Cordes, James M.; Cornish, Neil J.; Crawford, Fronefield; Cromartie, H. Thankful; Decesar, Megan E.; Demorest, Paul B.; Dolch, Timothy (2021-06-01). "The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc". The Astrophysical Journal. 914 (2): 121. arXiv: 2101.02716 . Bibcode:2021ApJ...914..121A. doi: 10.3847/1538-4357/abfcd3 . ISSN   0004-637X.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.