NGC 3751

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NGC 3751
N3750s-crop.jpg
NGC 3751 is located at the bottommost left of the image below NGC 3750, NGC 3753 and NGC 3754 which was taken by Mount Lemmon Observatory
Observation data
Constellation Leo
Right ascension 11h 37m 53.859s
Declination +21d 56m 11.34s
Redshift 0.031328
Heliocentric radial velocity 9,392 km/s
Distance 450 Mly (138 Mpc)
Group or cluster Copeland Septet
Apparent magnitude  (V)14.3
Characteristics
Type E4, E-S0
Size144,000 ly
Other designations
PGC 36017, UGC 6601, MCG +04-28-009, 2MASX J11375386+2156110, SDSS J113753.85+215611.3, Copeland Septet NED05, HCG 057F, NSA 112845, SSTSL2 J113753.87+215611.2, LEDA 36017

NGC 3751 is a type E-S0 [1] lenticular galaxy located in the Leo constellation. [2] It is located 450 million light-years away from the Solar System [3] and was discovered by Ralph Copeland on April 5, 1874. [4]

To date, a non-redshift measurement gives a distance of approximately 138,000 Mpc (450 million light-years) for NGC 3751. This value is within the Hubble Distance values. [5]

Copeland Septet

Sloan Digital Sky Survey of NGC 3751 NGC3751 - SDSS DR14.jpg
Sloan Digital Sky Survey of NGC 3751

NGC 3751 is a member of the Copeland Septet. [6] The other members are NGC 3745, NGC 3746, NGC 3748, NGC 3750, NGC 3753 and NGC 3754. [7]

Halton Arp noticed the 7 galaxies in which he published inside his article in 1966. [8] This group is known as Arp 320 in which another galaxy, PGC 36010 is part of it. [9]

This group was also observed by Paul Hickson, in which he included them inside his article which was published in 1982. [10] It is noted that this group is designated as Hickson 57. NGC 3751 is known as HCG 57F. [11]

Related Research Articles

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NGC 3718, also called Arp 214, is a galaxy located approximately 52 million light years from Earth in the constellation Ursa Major. It is either a lenticular or spiral galaxy.

<span class="mw-page-title-main">NGC 1190</span> Galaxy in the constellation Eridanus

NGC 1190 is a lenticular galaxy approximately 109 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 1189</span> Galaxy in the constellation Eridanus

NGC 1189 is a barred spiral galaxy approximately 105 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 1191</span> Galaxy in the constellation Eridanus

NGC 1191 is a lenticular galaxy approximately 406 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 1199</span> Galaxy in the constellation Eridanus

NGC 1199 is an elliptical galaxy approximately 107 million light-years away from Earth in the constellation of Eridanus. It was discovered by William Herschel on December 30, 1785.

<span class="mw-page-title-main">NGC 1192</span> Galaxy in the constellation Eridanus

NGC 1192 is a lenticular galaxy approximately 417 million light-years away from Earth in the constellation of Eridanus. It was discovered by American astronomer Francis Leavenworth on December 2, 1885 with the 26" refractor at Leander McCormick Observatory.

<span class="mw-page-title-main">NGC 508</span> Galaxy in the constellation Pisces

NGC 508, also occasionally referred to as PGC 5099 or UGC 939, is an elliptical galaxy in the constellation Pisces. It is located approximately 247 million light-years from the Solar System and was discovered on 12 September 1784 by British astronomer William Herschel.

<span class="mw-page-title-main">Copeland Septet</span> A group of galaxies in the constellation Leo

The Copeland Septet is a group of galaxies in the constellation Leo that includes NGC 3748, NGC 3754, NGC 3750, NGC 3751, NGC 3745, NGC 3753 and NGC 3746. The group was discovered by British astronomer Ralph Copeland in 1874. The location of Copeland's Septet is right ascension 11h 37m 50s / declination +21° 59′ (2000.0), about three degrees northwest of third magnitude star 93 Leonis.

<span class="mw-page-title-main">NGC 739</span> Galaxy in the constellation Triangulum

NGC 739 is a spiral galaxy approximately 193 million light-years away from Earth in the constellation of Triangulum.

<span class="mw-page-title-main">NGC 542</span> Galaxy in the constellation Andromeda

NGC 542 is a spiral galaxy in the constellation Andromeda, which is approximately 215 million light years from the Milky Way. Together with the galaxies NGC 529, NGC 531, and NGC 536, it forms the Hickson Compact Group 10, abbreviated HCG 10. It was discovered by Irish astronomer R.J. Mitchell in 1885.

<span class="mw-page-title-main">NGC 3746</span> Galaxy in the constellation Leo

NGC 3746 is a large barred spiral galaxy with a ring structure located in the Leo constellation. It is located 449 million light-years from the Solar System and has an approximate diameter of 165,000 light-years. NGC 3746 was discovered by Ralph Copeland on 9 February 1874 with subsequent observations made by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.

<span class="mw-page-title-main">NGC 3753</span> Galaxy in the constellation Leo

NGC 3753 is a large spiral galaxy with a bar located in the Leo constellation. It is located 435 million light-years away from the Solar System and was discovered on February 9, 1874, by Ralph Copeland.

<span class="mw-page-title-main">NGC 3750</span> Galaxy in the constellation Leo

NGC 3750 is a lenticular galaxy with a bar located in the constellation of Leo. It is located 450 million light-years from the Solar System and was discovered by Ralph Copeland on February 9, 1874.

<span class="mw-page-title-main">NGC 3748</span> Galaxy in the constellation Leo

NGC 3748 is a lenticular galaxy with a bar located in the Leo constellation. It is located 440 million light-years away from the Solar System and was discovered by Ralph Copeland on April 5, 1874, but also observed by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.

<span class="mw-page-title-main">NGC 3754</span> Galaxy in the constellation Leo

NGC 3754 is a small barred spiral galaxy located in Leo. It is located 447 million light-years away from the Solar System and was discovered on April 5, 1874, by Ralph Copeland.

<span class="mw-page-title-main">NGC 3745</span> Galaxy in the constellation Leo

NGC 3745 is a lenticular galaxy with a bar structure located in the constellation of Leo. NGC 3745 is located 471 million light-years away from the Solar System and was discovered by Ralph Copeland on April 5, 1874, but also observed by Hermann Kobold, Lawrence Parsons and John Louis Emil Dreyer.

<span class="mw-page-title-main">IC 2759</span> Elliptical galaxy in the constellation of Leo

IC 2759 is a small type E elliptical galaxy located in the constellation of Leo. It is located 350 million light-years away from the Solar System and was discovered on April 24, 1897, by Guillaume Bigourdan. Sometimes IC 2759 is confused with the spiral galaxy, PGC 34882 which is located south of the galaxy.

<span class="mw-page-title-main">NGC 3800</span> Galaxy in the constellation Leo

NGC 3800 is an intermediate spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 3,653 ± 24 km/s, which corresponds to a Hubble distance of 53.9 ± 3.8 Mpc. NGC 3800 was discovered by German-British astronomer William Herschel in 1784.

<span class="mw-page-title-main">NGC 3799</span> Galaxy in the constellation Leo

NGC 3799 is a barred spiral galaxy located in the constellation Leo. Its speed relative to the cosmic microwave background is 3,659 ± 24 km/s, which corresponds to a Hubble distance of 54.0 ± 3.8 Mpc. NGC 3799 was discovered by British astronomer John Herschel in 1832.

<span class="mw-page-title-main">NGC 7609</span> Galaxy in the constellation Pegasus

NGC 7609 or known as Arp 150 and HCG 95A, is a large elliptical galaxy located in Pegasus. Its speed relative to the cosmic microwave background is 11,879 km/s, which corresponds the galaxy to be located 554 million light-years away from Earth. NGC 7609 was discovered on October 5, 1864, by Albert Marth and included in Halton Arp's, Atlas of Peculiar Galaxies in galaxies that produces jets.

References

  1. ↑ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-05-03.
  2. ↑ Astronomy, Go. "NGC 3751 | galaxy in Leo | NGC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024-05-03.
  3. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-05-03.
  4. ↑ "New General Catalog Objects: NGC 3750 - 3799". cseligman.com. Retrieved 2024-05-03.
  5. ↑ "NED Distance Results for NGC 3751". ned.ipac.caltech.edu. Retrieved 2024-05-03.
  6. ↑ Bakich, Michael E. (2024-01-01). "Copeland's Septet". Astronomy Magazine. Retrieved 2024-05-03.
  7. ↑ "Copeland's Septet (Hickson Compact Group 57) – Constellation Guide". www.constellation-guide.com. Retrieved 2024-05-03.
  8. ↑ "NED Search Results for ARP 320". ned.ipac.caltech.edu. Retrieved 2024-05-03.
  9. ↑ "Copeland's Septet (Arp 320) - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-05-03.
  10. ↑ Hickson, P. (1982-04-01). "Systematic properties of compact groups of galaxies". The Astrophysical Journal. 255: 382–391. Bibcode:1982ApJ...255..382H. doi:10.1086/159838. ISSN   0004-637X.
  11. ↑ "Data from Revised NGC and IC catalogue by Wolfgang Steinicke - NGC 3700 to 3799". astrovalleyfield.ca. Retrieved 2024-05-03.
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