NGC 4546

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NGC 4546
NGC 4546 cutout hst 05446 2a wfpc2 total pc sci.jpg
NGC 4546 – Hubble Space Telescope – Hubble Legacy Archive
Observation data (J2000.0 epoch)
Constellation Virgo
Right ascension 12h 35m 29.5s [1]
Declination −03° 47′ 35.5″ [1]
Redshift 0.003492
Heliocentric radial velocity 1057 ± 5 km/s [1]
Distance 45.6 Mly
Apparent magnitude  (V)10.57 [1]
Characteristics
Type SB0− [1]
Other designations
PGC 41939, MCG-1-32-27, UGC 288

NGC 4546 is a lenticular field galaxy located in the direction of the constellation Virgo, [2] with a total population of globular clusters estimated at 390. [3] It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. [4]

Located 45.6 million light years away, with a stellar mass of about 27 billion solar masses, [1] it has a declination of −03° 47' 35" and an average rise of 12 hours, 35 minutes and 29.5 seconds. [5] NGC 4546 was discovered on December 29, 1786 by William Herschel. [6] [1] [3]

The galaxy appears to be home to a supermassive black hole with a mass of 256 million (± 16 million) times the mass of the Sun. [7] It is estimated to have 390±60 globular clusters. [8]

NGC 4546 appears to have at least 2 companions, [8] NGC 4546-UCD1 and CGCG 014-074. [8]

Related Research Articles

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Messier 84 or M84, also known as NGC 4374, is a giant elliptical or lenticular galaxy in the constellation Virgo. Charles Messier discovered the object in 1781 in a systematic search for "nebulous objects" in the night sky. It is the 84th object in the Messier Catalogue and in the heavily populated core of the Virgo Cluster of galaxies, part of the local supercluster.

<span class="mw-page-title-main">Messier 85</span> Elliptical galaxy in the constellation Coma Berenices

Messier 85 is a lenticular galaxy, or elliptical galaxy for other authors, in the Coma Berenices constellation. It is 60 million light-years away, and has a diameter of about 36.99 kiloparsecs across.

<span class="mw-page-title-main">NGC 4526</span> Lenticular galaxy in the constellation Virgo

NGC 4526 is a lenticular galaxy with an embedded dusty disc, located approximately 55 million light-years from the Solar System in the Virgo constellation and discovered on 13 April 1784 by William Herschel.

<span class="mw-page-title-main">NGC 4309</span> Galaxy in the constellation Virgo

NGC 4309 is a lenticular galaxy located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer Christian Peters in 1881 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4710</span> Galaxy in the constellation Coma Berenices

NGC 4710 is an edge-on lenticular galaxy in the northern constellation of Coma Berenices. It was discovered on March 21, 1784 by German-British astronomer William Herschel. This galaxy has a B-band visual magnitude of 11.60 and an angular size of 3.0′ × 0.8′. It is located at a distance of 54.5 ± 3.6 million light-years (16.7 ± 1.1 Mpc) from the Milky Way, and is receding with a heliocentric radial velocity of 1,129 km/s. This is a member of the Virgo Cluster, with a projected offset of ~6° from the cluster center and a cluster crossing time of around two billion years.

<span class="mw-page-title-main">NGC 3607</span> Galaxy in the constellation Leo

NGC 3607 is a small but fairly bright lenticular galaxy in the equatorial constellation of Leo, about 2.5° south of the prominent star Delta Leonis. The galaxy was discovered March 14, 1784 by William Herschel. Dreyer described it as "very bright, large, round, very much brighter middle, 2nd of 3". It is located at a distance of 73 million light years and is receding with a radial velocity of 930 km/s. The galaxy lies southwest of NGC 3626 at an angular separation of ~50′. It occupies the center of the Leo II Group of galaxies, forming one of its two brightest members – the other being NGC 3608. It is a member of the NGC 3607 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.

<span class="mw-page-title-main">NGC 4473</span> Galaxy in the constellation Coma Berenices

NGC 4473 is an elliptical galaxy located about 50 million light-years away in the constellation of Coma Berenices. It was discovered by astronomer William Herschel on April 8, 1784. NGC 4473 has an inclination of about 71°. NGC 4473 is a member of a chain of galaxies called Markarian's Chain which is part of the larger Virgo Cluster of galaxies.

<span class="mw-page-title-main">NGC 4753</span> Galaxy in the constellation Virgo

NGC 4753 is a lenticular galaxy located about 60 million light-years away in the constellation of Virgo. NGC 4753 was discovered by astronomer William Herschel on February 22, 1784. It is notable for having distinct dust lanes that surround its nucleus. It is a member of the NGC 4753 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.

<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 5084</span> Galaxy in the constellation Virgo

NGC 5084 is a lenticular galaxy in the constellation of Virgo. It is located at a distance of about 80 million light years from Earth, which, given its apparent dimensions, means that NGC 5084 is at least 200,000 light years across. It is one of the largest and most massive galaxies in the Virgo Supercluster. William Herschel discovered it on March 10, 1785. It is a member of the NGC 5084 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. The galaxy is seen nearly edge-on, with inclination 86°, and features a warped disk and large quantities of HI gas extending along the disk, probably accumulated after multiple accretions of smaller galaxies.

<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 1395</span> Galaxy in the constellation Eridanus

NGC 1395 is an elliptical galaxy located in the constellation Eridanus. It is located at a distance of circa 75 million light years from Earth, which, given its apparent dimensions, means that NGC 1395 is about 130,000 light years across. It was discovered by William Herschel on November 17, 1784. It is a member of the Eridanus Cluster.

<span class="mw-page-title-main">NGC 5982</span> Galaxy in the constellation Draco

NGC 5982 is an elliptical galaxy located in the constellation Draco. It is located at a distance of circa 130 million light years from Earth, which, given its apparent dimensions, means that NGC 5982 is about 100,000 light years across. It was discovered by William Herschel on May 25, 1788.

<span class="mw-page-title-main">NGC 1380</span> Galaxy in the constellation Fornax

NGC 1380 is a lenticular galaxy located in the constellation Fornax. It is located at a distance of circa 60 million light years from Earth, which, given its apparent dimensions, means that NGC 1380 is about 85,000 light years across. It was discovered by James Dunlop on September 2, 1826. It is a member of the Fornax Cluster.

<span class="mw-page-title-main">NGC 3585</span> Galaxy in the constellation Hydra

NGC 3585 is an elliptical or a lenticular galaxy located in the constellation Hydra. It is located at a distance of circa 60 million light-years from Earth, which, given its apparent dimensions, means that NGC 3585 is about 80,000 light years across. It was discovered by William Herschel on December 9, 1784.

<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 4365</span> Elliptical galaxy in the constellation Virgo

NGC 4365 is an elliptical galaxy located in the constellation Virgo. It was discovered by William Herschel on April 13, 1784.

<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 1373</span> Galaxy in the constellation Fornax

NGC 1373 is a dwarf elliptical galaxy located 61 millon light years away in constellation of Fornax. The galaxy was discovered by astronomer John Herschel on November 29, 1837, and is a member of the Fornax Cluster. NGC 1373 is a host to a supermassive black hole with an estimated mass of 4.6 millon solar masses.

<span class="mw-page-title-main">NGC 1396</span> Dwarf elliptical galaxy in the constellation of Fornax

NGC 1396 is a dwarf elliptical galaxy located 61 millon light years away in the constellation of Fornax. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster. Despite the fact that the galaxy PGC 13398 is most commonly identified as NGC 1396, there is uncertainty in its identification.

References

  1. 1 2 3 4 5 6 7 Escudero, C. G.; Faifer, F. R.; Castelli, A. V. Smith; Norris, M. A.; Forte, J. C. (2020-02-07). "Field/Isolated lenticular galaxies with high $S_N$ values: the case of NGC 4546 and its globular cluster system". Monthly Notices of the Royal Astronomical Society. 493 (2): 2253–2270. arXiv: 2002.02765 . Bibcode:2020MNRAS.493.2253E. doi: 10.1093/mnras/staa392 .
  2. ↑ Rojas, Sebastián García. "Galaxy NGC 4546 – Galaxy in Virgo Constellation". Telescopius. Retrieved 2020-02-18.
  3. 1 2 "Astronomers studied lenticular galaxy NGC 4546 in detail". Tech Explorist. 2020-02-18. Retrieved 2020-02-18.
  4. ↑ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
  5. ↑ Ford, Dominic. "The galaxy NGC 4546 − In-The-Sky.org". in-the-sky.org. Retrieved 2020-02-18.
  6. ↑ "NGC 4546 – Galaxy – SKY-MAP". server7.sky-map.org. Retrieved 2020-02-18.
  7. ↑ Ricci, T V; Steiner, J E (21 May 2020). "Measuring the mass of the supermassive black hole of the lenticular galaxy NGC 4546". Monthly Notices of the Royal Astronomical Society. 495 (3): 2620–2629. arXiv: 2005.13697 . doi: 10.1093/mnras/staa1398 . Retrieved 29 June 2020.
  8. 1 2 3 Escudero, Carlos G; Faifer, Favio R; Castelli, Analía V Smith; Norris, Mark A; Forte, Juan C (April 2020). "Field/isolated lenticular galaxies with high SN values: the case of NGC 4546 and its globular cluster system". Monthly Notices of the Royal Astronomical Society. 493 (2): 2253–2270. arXiv: 2002.02765 . Bibcode:2020MNRAS.493.2253E. doi: 10.1093/mnras/staa392 . Retrieved 29 June 2020.
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