IC 3505

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IC 3505
IC3505 - SDSS DR14.jpg
IC 3505 captured by Sloan Digital Sky Survey
Observation data
Constellation Coma Berenices
Right ascension 188.54 degrees
Declination 15.96 degrees
Redshift 0.04609 0.00001
Heliocentric radial velocity 13,843 km/s
Distance 645 Mly (197.8 Mpc)
Apparent magnitude  (V)12.412
Characteristics
Type SBc
Size170,000 ly
Other designations
IRAS 12316+1614, MCG+03-032-070, PGC 41792, 2MASX J12341031+1558058, VCC 1542, GASS 30439, ALFAFFA 1-349, AGC 220790, NVSS J123410+155803, LEDA 41792

IC 3505 is a barred spiral galaxy [1] located 640 million light-years [2] away from the Solar System in the Coma Berenices constellation. [3] With an apparent size of 0.95 by 0.35 arcmin, IC 3505 has an estimated diameter of 170,000 light-years, making it slightly larger compared to the Milky Way. [2] It is categorized as a LINER galaxy [4] with an active galactic nucleus [5] emitting weak emission-lines. [6]

IC 3505 was discovered by Royal Harwood Frost on May 7, 1904. [7] According to Frost when he saw the object for the first time, he listed it as a type SBc at right ascension "12 34 10.3" and declination "+15 58 07". [7] Despite being listed in the Virgo Cluster catalogue as VCC 1542, it is not part of the Virgo Cluster but a background galaxy. [8]

Two supernovae have been discovered in IC 3505. SN 2019iaz (Type Ia, mag: 19.6) was discovered on June 21, 2019, by C. Fremling from Caltech on behalf on Zwicky Transient Facility (ZTF) [9] and AT 2023gpz (unknown, mag: 20.2) which was discovered by K. De (also from ZTF) on April 21, 2023. [10]

Related Research Articles

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NGC 4457 is an intermediate spiral galaxy located about 55 million light-years away in the constellation of Virgo. It is also classified as a LINER galaxy, a class of active galaxy defined by their spectral line emissions. NGC 4457 Is inclined by about 33°. It was discovered by astronomer William Herschel on February 23, 1784. Despite being listed in the Virgo Cluster Catalog as VCC 1145, NGC 4457 is a member of the Virgo II Groups which form an extension of the Virgo cluster.

<span class="mw-page-title-main">NGC 3861</span> Galaxy in the constellation Leo

NGC 3861 is a large barred spiral galaxy with a ring-like structure located about 310 million light-years away in the constellation Leo. It was discovered by astronomer John Herschel on March 23, 1827. NGC 3861 is a member of the Leo Cluster and has a normal amount of neutral hydrogen and ionised hydrogen.

<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 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 4076</span> Galaxy in the constellation Coma Berenices

NGC 4076 is a spiral galaxy located 290 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 27, 1785 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4307</span> Spiral galaxy in the constellation Virgo

NGC 4307 is an edge-on spiral galaxy located about 65 million light-years away in the constellation Virgo. It was discovered by astronomer Christian Peters in 1881 and is a member of the Virgo Cluster. It is also a LINER galaxy.

<span class="mw-page-title-main">NGC 4316</span> Spiral galaxy in the constellation Virgo

NGC 4316 is an edge-on spiral galaxy located about 70 million light-years away in the constellation Virgo. It was discovered by astronomer Wilhelm Tempel on March 17, 1882. NGC 4316 is a member of the Virgo Cluster and is classified as LINER and as a Seyfert galaxy.

<span class="mw-page-title-main">NGC 4333</span> Barred spiral galaxy in the constellation Virgo

NGC 4333 is a barred spiral galaxy with a ring structure located about 330 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784, who described it as "F, pS, R, bM, 2nd of 3". NGC 4333 is also classified as a LINER galaxy. Despite being listed in the Virgo Cluster catalog as VCC 637, it is not a member of the Virgo Cluster but instead a background galaxy.

<span class="mw-page-title-main">IC 3528</span> Galaxy in the constellation Coma Berenices

IC 3528 is a Seyfert 1.5 type spiral galaxy with X-ray emission located 660 million light-years away in the constellation of Coma Berenices. It lies near to spiral galaxy NGC 4540, although the two of them are quite far. The object was discovered by Royal Harwood Frost on May 7, 1904. Although listed as a member in the Virgo Cluster Catalogue as VCC 1593, it is not a member of the Virgo cluster but a background galaxy.

<span class="mw-page-title-main">IC 3053</span> Galaxy in the constellation Coma Berenices

IC 3053 is a type Sab barred spiral galaxy with a ring located in the Coma Berenices constellation. The galaxy lies 720 million light-years from the Solar System and has an estimated diameter of 180,000 light-years meaning the galaxy is much larger compared to the Milky Way. IC 3053 was first discovered by Royal Harwood Frost on May 7, 1904. Despite listed in the Virgo Cluster Catalogue as VCC 95, it is not a member of the Virgo Cluster due to its high redshift and instead a background galaxy.

<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.

<span class="mw-page-title-main">IC 4040</span> Galaxy in the constellation Coma Berenices

IC 4040 is a type SABc spiral galaxy with a bar in Coma Berenices. It is located 353 million light-years away from the Solar System and has an estimated diameter of 105,000 light-years making it slightly larger than the Milky Way. IC 4040 was discovered on April 12, 1891, by Guillaume Bigourdan and is a member of the Coma Cluster.

<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">IC 5145</span>

IC 5145 is a type Sab spiral galaxy located in the constellation Pegasus. It is located 356 million light-years from the Solar System and was discovered by Edward Emerson Barnard, although the year he discovered it is unknown.

<span class="mw-page-title-main">NGC 7222</span> Large barred spiral galaxy with a ring structure

NGC 7222 is a large barred spiral galaxy with a ring structure, located in the constellation Aquarius. It is located 570 million light-years away from the Solar System and was discovered by German astronomer, Albert Marth on August 11, 1864.

<span class="mw-page-title-main">IC 3275</span>

IC 3275 is a spiral galaxy with a ring structure located in the Virgo constellation. It is located 811 million light-years away from the Solar System and has an approximate diameter of 120,000 light-years across. IC 3275 was discovered on May 7, 1904, by Royal Harwood Frost.

<span class="mw-page-title-main">IC 2498</span>

IC 2498 known as PGC 27668, is a type Sb barred spiral galaxy located in constellation Leo. It is located 469 million light-years away from the Solar System and was discovered by Stephane Javelle on April 30, 1896.

<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">IC 1050</span>

IC 1050 is a type Sbc spiral galaxy located in constellation Boötes. It is located 491 million light-years from the Solar System and has an approximate diameter of 130,000 light-years. IC 1050 was discovered by Stephane Javelle on June 3, 1892.

<span class="mw-page-title-main">IC 4588</span>

IC 4588 is a type E elliptical galaxy located in the constellation Serpens. It is located 729 million light-years from the Solar System and has a dimension of 0.30 x 0.3 arcmin meaning its diameter is 64,000 light-years across. IC 4588 was discovered by Stephane Javelle on July 15, 1903.

References

  1. ↑ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024-04-22.
  2. 1 2 "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-22.
  3. ↑ "IC 3505". spider.seds.org. Retrieved 2024-04-22.
  4. ↑ Larkin, J. E.; Armus, L.; Knop, R. A.; Soifer, B. T.; Matthews, K. (1998-01-01). "A Near-Infrared Spectroscopic Survey of LINER Galaxies". The Astrophysical Journal Supplement Series. 114 (1): 59. arXiv: astro-ph/9708097 . Bibcode:1998ApJS..114...59L. doi:10.1086/313063. ISSN   0067-0049.
  5. ↑ Márquez, Isabel; Masegosa, Josefa; González-Martin, Omaira; Hernández-Garcia, Lorena; Pović, Mirjana; Netzer, Hagai; Cazzoli, Sara; del Olmo, Ascensión (2017). "The AGN Nature of LINER Nuclear Sources". Frontiers in Astronomy and Space Sciences. 4: 34. Bibcode:2017FrASS...4...34M. doi: 10.3389/fspas.2017.00034 . ISSN   2296-987X.
  6. ↑ Heckman, T. M. (1980-07-01). "An Optical and Radio Survey of the Nuclei of Bright Galaxies - Activity in the Normal Galactic Nuclei". Astronomy and Astrophysics. 87: 152. Bibcode:1980A&A....87..152H. ISSN   0004-6361.
  7. 1 2 "Index Catalog Objects: IC 3500 - 3549". cseligman.com. Retrieved 2024-04-22.
  8. ↑ Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo cluster. II. A catalog of 2096 galaxies in the Virgo cluster area". The Astronomical Journal. 90: 1681–1758. Bibcode:1985AJ.....90.1681B. doi:10.1086/113874. ISSN   0004-6256.
  9. ↑ "SN 2019iaz | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-05.
  10. ↑ "AT 2023gpz | Transient Name Server". www.wis-tns.org. Retrieved 2024-05-05.
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