UGC 4653

Last updated
UGC 4653
Squabbling Galactic Siblings.jpg
Hubble Space Telescope image of UGC 4653
Observation data (J2000 epoch)
Constellation Lynx
Right ascension 08h 53m 54.6s
Declination +35° 09′ 00″
Redshift 0.056836
Heliocentric radial velocity 16,748 km/s
Distance 763 Mly (233.9 Mpc)
Apparent magnitude  (V)0.093
Apparent magnitude  (B)0.124
Characteristics
Type SB(s)b
Apparent size  (V)1.9' x 1.1'
Notable featuresInteracting galaxy
Other designations
PGC 24981, SDSS J085354.62+350844.0, 2MASX J08535462+3508439, Arp 195, LEDA 24981, MCG+06-20-012, VV 243

UGC 4653 known as Arp 195, is a trio of interacting galaxies located 763 million light-years away from the solar system in the Lynx constellation. [1] The galaxies are being distorted through gravitational interactions with each other. [2] [3] The first known reference for this object, was in 1959 where B.A. Vorontsov-Vel'yaminov compiled it inside the Vorontsov-Vel'yaminov Interacting galaxies, as VV 243. [4]

This image of UGC 4653 was captured by the Hubble Space Telescope. [2] The galaxies make up the 195th object in the Atlas of Peculiar Galaxies created by Halton Arp. [5] They fall into the category of galaxies with material ejected from nuclei. [6]

UGC 4653 has active nuclear regions which produce infrared (IR) emissions. [7] These appear to be more like AGNs than HII regions. [7]

A study published in 2023, confirmed all three galaxies of the UGC 4653 system are spirals. The southern galaxy is a face-on galaxy hosting a bright core, while the central is edge-on but no clear distinction whether it is an early or late-type galaxy. The northern galaxy has a tidal tail and is of late-type morphology. With the exception of the third, both galaxies contain presence of strong emission lines. [8]

Supernova

Type Ia supernova, SN 2008bv [9] was discovered in UGC 4653 with a magnitude of 18.3. [10] It was located 1".7 east and 3".9 south of the nucleus. [11]

Related Research Articles

<span class="mw-page-title-main">NGC 3432</span> Galaxy in the constellation Leo Minor

NGC 3432 is an edge-on spiral galaxy that can be found in the northern constellation of Leo Minor. It was discovered by German-British astronomer William Herschel on March 19, 1787. This galaxy is located at a distance of 40 million light-years (12.3 Mpc) from the Milky Way. It is interacting with UGC 5983, a nearby dwarf galaxy, and features tidal filaments and intense star formation. Because of these features, it was listed in Halton Arp's Atlas of Peculiar Galaxies.

<span class="mw-page-title-main">NGC 935 and IC 1801</span> Pair of interacting galaxies in the constellation Aries

NGC 935 and IC 1801 are a pair of interacting galaxies within the Aries constellation. They were discovered on 18 September 1885 by Lewis Swift. NGC 935 is the northern member of the pair, and IC 1801 is the southern. Together, they are listed in Halton Arp's Atlas of Peculiar Galaxies as Arp 276, as an example of interacting galaxies.

<span class="mw-page-title-main">UGC 9425</span> Interacting galaxies in the constellation Boötes

UGC 9425 are a pair of interacting galaxies located in the constellation of Boötes, comprising PGC 52283 and PGC 87675, both disk-type galaxies. It is located 468 million light-years from Earth and catalogued as Arp 241 by Halton Arp.

<span class="mw-page-title-main">NGC 5829</span> Galaxy in the constellation Boötes

NGC 5829 is a spiral galaxy located in the constellation Boötes. It is 281 million light-years away from Earth and was discovered by astronomer, Edouard Stephan in May 1882.

<span class="mw-page-title-main">Arp 273</span> Pair of interacting galaxies in the constellation Andromeda

Arp 273 is a pair of interacting galaxies, 300 million light years away in the constellation Andromeda. It was first described in the Atlas of Peculiar Galaxies, compiled by Halton Arp in 1966. The larger of the spiral galaxies, known as UGC 1810, is about five times more massive than the smaller galaxy. It has a disc that is tidally distorted into a rose-like shape by the gravitational pull of the companion galaxy below it, known as UGC 1813. The smaller galaxy shows distinct signs of active star formation at its nucleus, and "it is thought that the smaller galaxy has actually passed through the larger one."

<span class="mw-page-title-main">NGC 6040</span> Galaxy in the constellation Hercules

NGC 6040 is a spiral galaxy located about 550 million light-years away in the constellation Hercules. NGC 6040 was discovered by astronomer Édouard Stephan on June 27, 1870. NGC 6040 is interacting with the lenticular galaxy PGC 56942. As a result of this interaction, NGC 6040's southern spiral arm has been warped in the direction toward PGC 56942. NGC 6040 and PGC 56942 are both members of the Hercules Cluster.

<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 4302</span> Galaxy in the constellation Coma Berenices

NGC 4302 is an edge-on spiral galaxy located about 55 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 8, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">Arp 146</span> Interacting galaxies in the constellation Cetus

Arp 146 are a pair of interacting galaxies located 1.05 billion light-years away from Earth in the Cetus constellation. It was discovered by Dewhirst and catalogued by Boris Vorontsov-Velyaminov as VV 790. Under the Atlas of Peculiar Galaxies created by Halton Arp, they are categorized under galaxies that have associated rings.

<span class="mw-page-title-main">UGC 934</span> Galaxy in the constellation Pisces

UGC 934, known as PGC 5085, is a large spiral galaxy about 470 million light-years away from the solar system. It is located in the constellation of Pisces and about 285,000 thousand light-years in diameter.

<span class="mw-page-title-main">UGC 4881</span> Peculiar galaxies in the constellation Lynx

UGC 4881 is a pair of interacting galaxies, UGC 4881A and UGC 4881B. They are located in the constellation Lynx, some 500 million light-years away. UGC 4881, the brighter, is a peculiar spiral galaxy. It has been heavily documented by the Hubble Space Telescope, and is cataloged in the Atlas of Peculiar Galaxies.

<span class="mw-page-title-main">UGC 1840</span> Interacting galaxies in the constellation Andromeda

UGC 1840, also known as Arp 145, are a pair of interacting galaxies located 250 million light-years away from the Solar System in the Andromeda constellation. The earliest known reference to the pair of galaxies is in part 2 of the Morphological Catalogue of Galaxies, published in 1964, where it is listed as MCG +07-06-002.

<span class="mw-page-title-main">UGC 6697</span> Galaxy in the constellation Leo

UGC 6697 is a large irregular spiral galaxy with a bar located in the Leo constellation. It is located 378 million light-years from the Solar System and has an estimated diameter of 205,000 light-years. UGC 6697 is considered a starburst galaxy which produces high rates of star formation. The first known reference to this galaxy comes from volume II of the Catalogue of Galaxies and of Clusters of Galaxies compiled by Fritz Zwicky in 1968, where it was listed as CGCG 097-087, and its coordinates listed as 1141.2 + 2015.

<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 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">NGC 3751</span> Galaxy in the constellation Leo

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

<span class="mw-page-title-main">NGC 3509</span> Galaxy in the constellation Leo

NGC 3509 known as Arp 335, is a barred spiral galaxy located in the constellation Leo. It is located 340 million light-years from the Solar System. NGC 3509 was discovered by astronomer William Herschel on December 30, 1786.

<span class="mw-page-title-main">UGC 9684</span> Galaxy located in Boötes

UGC 9684 is a barred spiral galaxy with a ring structure in the Boötes constellation. It is located 250 million light-years from the Solar System and has an approximate diameter of 90,000 light-years.

<span class="mw-page-title-main">NGC 4017</span> Spiral radio galaxy in the constellation Coma Berenices

NGC 4017 is an intermediate spiral radio galaxy located in the constellation Coma Berenices. Its speed relative to the cosmic microwave background is 3,748 ± 21 km/s, which corresponds to a Hubble distance of 55.3 ± 3.9 Mpc. NGC 4017 was discovered by German-British astronomer William Herschel in 1785.

<span class="mw-page-title-main">NGC 5394</span> Interacting barred spiral galaxy in the constellation Canes Venatici

NGC 5394 is a barred spiral galaxy located in the constellation Canes Venatici. Its speed relative to the cosmic microwave background is 3,639 ± 14 km/s, which corresponds to a Hubble distance of 53.7 ± 3.8 Mpc. NGC 5394 was discovered by German-British astronomer William Herschel in 1787.

References

  1. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-21.
  2. 1 2 information@eso.org. "Squabbling Galactic Siblings". www.spacetelescope.org. Retrieved 2024-04-21.
  3. ↑ Ryan, C. J.; De Robertis, M. M. (2010-01-21). "The Local Environments of Interacting Galaxy Systems". The Astrophysical Journal. 710 (1): 783–796. Bibcode:2010ApJ...710..783R. doi:10.1088/0004-637x/710/1/783. ISSN   0004-637X.
  4. ↑ Vorontsov-Velyaminov, B.A. "The Atlas and Catalogue of Interacting Galaxies Part 1". ned.ipac.caltech.edu. Retrieved 2024-09-09.
  5. ↑ "Halton Arp's Atlas of Peculiar Galaxies". cseligman.com. Retrieved 2024-04-21.
  6. ↑ "Arp 195 - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-04-21.
  7. 1 2 Fiorenza, Stephanie; Uzan, Raphael (2019). "A Study of the Nuclear Regions of the Triple Merging System Arp 195". American Astronomical Society Meeting Abstracts #233. 233. Bibcode:2019AAS...23317302F . Retrieved 27 April 2024.
  8. ↑ Misquitta, Persis; Eckart, Andreas; Zajaček, Michal; Yttergren, Madeleine (March 2023). "SDSS-FIRST-selected interacting galaxies". Astronomy & Astrophysics. 671: A18. doi: 10.1051/0004-6361/202244721 . ISSN   0004-6361.
  9. ↑ Li, W.; Filippenko, A. V. (2008-04-01). "Supernova 2008bv in UGC 4653". Central Bureau Electronic Telegrams. 1345: 1. Bibcode:2008CBET.1345....1L.
  10. ↑ "Bright Supernovae - 2008". www.rochesterastronomy.org. Retrieved 2024-04-21.
  11. ↑ "SN 2008bv". w.astro.berkeley.edu. Retrieved 2024-04-21.
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