Astronomy:Markarian 273

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Short description: Galaxy in the constellation of Ursa Major
Markarian 273
Hubble Interacting Galaxy Mrk 273 (2008-04-24).jpg
Mrk 273 by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension 13h 44m 42.1s[1]
Declination+55° 53′ 13″[1]
Redshift0.037340 ± 0.000008 [1]
Helio radial velocity11,194 ± 2 km/s[1]
Distance502 Mly (154 Mpc)[1]
Apparent magnitude (V)14.8
Characteristics
TypePec [1]
Apparent size (V)0.72′ × 0.40′[1]
Notable featuresUltraluminour infrared galaxy, Seyfert galaxy
Other designations
UGC 8696, VV 851, I Zw 071, MCG +09-23-004, PGC 48711[1]

Markarian 273 is a galaxy merger located in the constellation Ursa Major. It is located at a distance of about 500 million light years from Earth, which, given its apparent dimensions, means that Markarian 273 is about 130,000 light years across.[1] It is an ultraluminous infrared galaxy and a Seyfert galaxy.

Characteristics

Markarian 273 is a galaxy merger, the result of two or more galaxies colliding. When observed in mid infrared, two nuclei are visible, with a projected separation of about 0.75 kiloparsec.[2] The southwest nucleus is known to be active, due its X-ray emission,[3] while the northeast nucleus too displays a heavily abosrbed X-ray spectrum, indicating that is also active.[2] The optical emission of the southwest nucleus corresponds to a type II Seyfert galaxy while the north one of a LINER.[4] A third component in the nuclear region is visible at the southeast in the radiowaves and could be a star cluster.[3]

The galaxy experiences a starburst, with a star formation rate of 139 M☉ per year.[5] This activity makes the galaxy shine bright in the infrared and it is categorised as ultra-luminous infrared galaxy, with total infrared luminosity of the galaxy is estimated to be 1012.1 L☉.[6] The startburst takes place in a rotating disk with a radius 120 pc and a total mass of 2.6×109 M☉ which surrounds the north nucleus.[7] It has been suggested that this is the location of compact luminous supernovae remnants and radio supernovae.[8] The startburst is fed by large amounts of cold molecular gas. The gas has complex kinematics due to the presence of outflows. A kiloparsec scale outflow is visible towards the north in CO imaging, with the flow rate of 600 M☉ per year.[5] The outflows reach about 5 kpc from the nucleus.[9] There is also evidence of a bipolar superbubble.[10]

The merger has a tidal tail extending southwards for 40 kiloparsecs, that is seen edge on.[3] Also south of the galaxy lies a giant X-ray nebula, measuring 40 by 40 kiloparsecs in size, that isn't closely related with the tidal tail. The gas temperature of the nebula is estimated to be 7 million K, possibly heated by galactic outflows.[2] Filaments and clumps of ionised gas visible in OIII are extending about 23 kpc to the east.[11] A warm gas ionised halo extends about 45 kpc from the nucleus, and is probably tidal debris from the merger.[12] When observed in radiowaves the galaxy has two large plumes, one to the south, extending to about 100 kpc, and one dimmer to the north, extending to about 190 kpc.[13]

See also

  • Arp 220 - the closest ultraluminous infrared galaxy to Earth
  • NGC 6240 - galaxy merger and ultraluminous infrared galaxy

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 "NASA/IPAC Extragalactic Database". Results for MRK 273. http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=MRK+273. 
  2. ↑ 2.0 2.1 2.2 Liu, Weizhe; Veilleux, Sylvain; Iwasawa, Kazushi; Rupke, David S. N.; Teng, Stacy; U, Vivian; Tombesi, Francesco; Sanders, David et al. (8 February 2019). "Elliptical Galaxy in the Making: The Dual Active Galactic Nuclei and Metal-enriched Halo of Mrk 273". The Astrophysical Journal 872 (1): 39. doi:10.3847/1538-4357/aafdfc. Bibcode: 2019ApJ...872...39L. 
  3. ↑ 3.0 3.1 3.2 Iwasawa, K.; Mazzarella, J. M.; Surace, J. A.; Sanders, D. B.; Armus, L.; Evans, A. S.; Howell, J. H.; Komossa, S. et al. (April 2011). "The location of an active nucleus and a shadow of a tidal tail in the ULIRG Mrk 273". Astronomy & Astrophysics 528: A137. doi:10.1051/0004-6361/201015872. Bibcode: 2011A&A...528A.137I. 
  4. ↑ Colina, Luis; Arribas, Santiago; Borne, Kirk D. (10 December 1999). "Integral Field Spectroscopy of Markarian 273: Mapping High-Velocity Gas Flows and an Off-Nucleus Seyfert 2 Nebula". The Astrophysical Journal 527 (1): L13–L16. doi:10.1086/312389. PMID 10566988. Bibcode: 1999ApJ...527L..13C. 
  5. ↑ 5.0 5.1 Cicone, C.; Maiolino, R.; Sturm, E.; Graciá-Carpio, J.; Feruglio, C.; Neri, R.; Aalto, S.; Davies, R. et al. (February 2014). "Massive molecular outflows and evidence for AGN feedback from CO observations". Astronomy & Astrophysics 562: A21. doi:10.1051/0004-6361/201322464. Bibcode: 2014A&A...562A..21C. 
  6. ↑ Kim, D.-C.; Veilleux, S.; Sanders, D. B. (December 2002). "Optical and Near-Infrared Imaging of the IRAS 1 Jy Sample of Ultraluminous Infrared Galaxies. I. The Atlas". The Astrophysical Journal Supplement Series 143 (2): 277–314. doi:10.1086/343843. Bibcode: 2002ApJS..143..277K. 
  7. ↑ Downes, D.; Solomon, P. M. (10 November 1998). "Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies". The Astrophysical Journal 507 (2): 615–654. doi:10.1086/306339. Bibcode: 1998ApJ...507..615D. 
  8. ↑ Bondi, M.; Pérez-Torres, M-A.; Dallacasa, D.; Muxlow, T. W. B. (September 2005). "A supernova factory in Mrk 273?". Monthly Notices of the Royal Astronomical Society 361 (2): 748–752. doi:10.1111/j.1365-2966.2005.09206.x. Bibcode: 2005MNRAS.361..748B. 
  9. ↑ Leung, Gene C. K.; Coil, Alison L.; Rupke, David S. N.; Perrotta, Serena (1 June 2021). "KCWI Observations of the Extended Nebulae in Mrk 273". The Astrophysical Journal 914 (1): 17. doi:10.3847/1538-4357/abf4da. Bibcode: 2021ApJ...914...17L. 
  10. ↑ Rupke, David S. N.; Veilleux, Sylvain (16 April 2013). "The Multiphase Structure and Power Sources of Galactic Winds in Major Mergers". The Astrophysical Journal 768 (1): 75. doi:10.1088/0004-637X/768/1/75. Bibcode: 2013ApJ...768...75R. 
  11. ↑ Rodríguez Zaurín, J.; Tadhunter, C. N.; Rupke, D. S. N.; Veilleux, S.; Spoon, H. W. W.; Chiaberge, M.; Ramos Almeida, C.; Batcheldor, D. et al. (November 2014). "Extended warm gas in the ULIRG Mrk273: Galactic outflows and tidal debris". Astronomy & Astrophysics 571: A57. doi:10.1051/0004-6361/201423540. Bibcode: 2014A&A...571A..57R. 
  12. ↑ Spence, R. A. W.; Zaurín, J. Rodríguez; Tadhunter, C. N.; Rose, M.; Cabrera-Lavers, A.; Spoon, H.; Muñoz-Tuñón, C. (11 June 2016). "No evidence for large-scale outflows in the extended ionized halo of ULIRG Mrk273". Monthly Notices of the Royal Astronomical Society: Letters 459 (1): L16–L20. doi:10.1093/mnrasl/slw033. 
  13. ↑ Kukreti, P.; Morganti, R.; Bondi, M.; Oosterloo, T.; Tadhunter, C.; Morabito, L. K.; Adams, E. A. K.; Adebahr, B. et al. (August 2022). "Seeing the forest and the trees: A radio investigation of the ULIRG Mrk 273". Astronomy & Astrophysics 664: A25. doi:10.1051/0004-6361/202243174. Bibcode: 2022A&A...664A..25K. 

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