Astronomy:IC 3505
| IC 3505 | |
|---|---|
 IC 3505 captured by Sloan Digital Sky Survey | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 34m 10.31s |
| Declination | +15° 58′ 05.60″ |
| Redshift | 0.046090 |
| Helio radial velocity | 13,843 km/s |
| Distance | 645 Mly (197.8 Mpc) |
| Apparent magnitude (V) | 12.412 |
| Characteristics | |
| Type | SBc |
| Size | 170,000 ly |
| Apparent size (V) | 1.01' x 0.41' |
| 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]
References
- ↑ "HyperLeda -object description". http://atlas.obs-hp.fr/hyperleda/ledacat.cgi?o=IC%203505.
- ↑ 2.0 2.1 "Your NED Search Results". https://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Obj_id&objid=30971&objname=1&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1.
- ↑ "IC 3505". https://spider.seds.org/ngc/ngc.cgi?CatalogNumber=IC+3505.
- ↑ Larkin, J. E.; Armus, L.; Knop, R. A.; Soifer, B. T.; Matthews, K. (1998-01-01). "A Near-Infrared Spectroscopic Survey of LINER Galaxies" (in en). The Astrophysical Journal Supplement Series 114 (1): 59. doi:10.1086/313063. ISSN 0067-0049. Bibcode: 1998ApJS..114...59L. https://iopscience.iop.org/article/10.1086/313063/meta.
- ↑ 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. doi:10.3389/fspas.2017.00034. ISSN 2296-987X. Bibcode: 2017FrASS...4...34M.
- ↑ 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. ISSN 0004-6361. Bibcode: 1980A&A....87..152H. https://ui.adsabs.harvard.edu/abs/1980A&A....87..152H.
- ↑ 7.0 7.1 "Index Catalog Objects: IC 3500 - 3549". https://cseligman.com/text/atlas/ic35.htm#ic3505.
- ↑ 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. doi:10.1086/113874. ISSN 0004-6256. Bibcode: 1985AJ.....90.1681B. https://ui.adsabs.harvard.edu/abs/1985AJ.....90.1681B.
- ↑ "SN 2019iaz | Transient Name Server". https://www.wis-tns.org/object/2019iaz.
- ↑ "AT 2023gpz | Transient Name Server". https://www.wis-tns.org/object/2023gpz.
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