Astronomy:Messier 77

From HandWiki
Short description: Barred spiral galaxy in the constellation Cetus
Messier 77
Messier 77 spiral galaxy by HST.jpg
Observation data (J2000 epoch)
ConstellationCetus
Right ascension 02h 42m 40.771s[1]
Declination−00° 00′ 47.84″[1]
Redshift1,137±3 km/s[2]
Distance47 Mly (14.4 Mpc)[3]
Apparent magnitude (V)8.9[4]
Characteristics
Type(R)SA(rs)b[5]
Mass~1×109[6] M☉
Apparent size (V)7.1′ × 6.0′[2]
Notable featuresOne of the biggest galaxies of Messier's catalog. Inclination estimated to be 40°.[3]
Other designations
Cetus A, M77, NGC 1068, 3C 71, 4C -00.13, Arp 37, UGC 2188, PGC 10266[7]

Messier 77 (M77), also known as NGC 1068 or the Squid Galaxy, is a barred spiral galaxy in the constellation Cetus. It is about 47 million light-years (14 Mpc) away from Earth. Messier 77 was discovered by Pierre Méchain in 1780, who originally described it as a nebula. Méchain then communicated his discovery to Charles Messier, who subsequently listed the object in his catalog.[8] Both Messier and William Herschel described this galaxy as a star cluster.[8] Today, however, the object is known to be a galaxy.

The morphological classification of NGC 1068 in the De Vaucouleurs system is (R)SA(rs)b,[5] where the '(R)' indicates an outer ring-like structure, 'SA' denotes a non-barred spiral, '(rs)' means a transitional inner ring/spiral structure, and 'b' says the spiral arms are moderately wound.[9] Ann et al. (2015) gave it a class of SAa,[10] suggesting tightly wound arms. However, infrared images of the inner part of the galaxy reveal a prominent bar not seen in visual light,[11] and for this reason it is now considered a barred spiral.[12]

Messier 77 is an active galaxy with an active galactic nucleus (AGN), which is obscured from view by astronomical dust at visible wavelengths. The diameter of the molecular disk and hot plasma associated with the obscuring material was first measured at radio wavelengths by the VLBA and VLA. The hot dust around the nucleus was subsequently measured in the mid-infrared by the MIDI instrument at the VLTI. It is the brightest[13] and one of the closest and best-studied[12] type 2 Seyfert galaxies,[3] forming a prototype of this class.[12]

M77 Type II Supernova, November 2018

X-ray source 1H 0244+001 in Cetus has been identified as Messier 77.[14] Only one supernova has been detected in Messier 77. The supernova, named SN 2018ivc, was discovered on 24 November 2018 by the DLT40 Survey. It is a type II supernova, and at discovery it was 15th magnitude and brightening.[15]

In February 2022 the European Southern Observatory found a cloud of cosmic dust at the centre of Messier 77 hiding a supermassive black hole.[16]

In November 2022, the IceCube collaboration announced the detection of a neutrino source emitted by the active galactic nucleus of Messier 77.[17][18] It is the second detection by IceCube after TXS 0506+056, and only the fourth known source including SN1987A and solar neutrinos.

See also

References

  1. ↑ 1.0 1.1 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W. et al. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal 131 (2): 1163–1183. doi:10.1086/498708. ISSN 0004-6256. Bibcode: 2006AJ....131.1163S. https://ui.adsabs.harvard.edu/abs/2006AJ....131.1163S/abstract. 
  2. ↑ 2.0 2.1 "NASA/IPAC Extragalactic Database". Results for NGC 1068. http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=m77&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES. 
  3. ↑ 3.0 3.1 3.2 R. J. Rand; J. F. Wallin (2004). "Pattern Speeds BIMA-SONG Galaxies with Molecule-Dominated ISMs Using the Tremaine-Weinberg Method". The Astrophysical Journal 614 (1): 142–157. doi:10.1086/423423. Bibcode: 2004ApJ...614..142R. 
  4. ↑ "Messier 77". https://messier.seds.org/m/m077.html. 
  5. ↑ 5.0 5.1 de Vaucouleurs, G. et al. (1991), Third reference catalogue of bright galaxies, 9, New York: Springer-Verlag. 
  6. ↑ "Messier 77: Cetus A - Messier Objects". 24 July 2015. http://www.messier-objects.com/messier-77-cetus-a/. 
  7. ↑ "M 77". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=M+77. 
  8. ↑ 8.0 8.1 K. G. Jones (1991). Messier's Nebulae and Star Clusters (2nd ed.). Cambridge University Press. ISBN 978-0-521-37079-0. 
  9. ↑ de Vaucouleurs, Gérard (April 1963), "Revised Classification of 1500 Bright Galaxies", Astrophysical Journal Supplement 8: 31, doi:10.1086/190084, Bibcode: 1963ApJS....8...31D. 
  10. ↑ Ann, H. B. et al. (2015), "A Catalog of Visually Classified Galaxies in the Local (z ~ 0.01) Universe", The Astrophysical Journal Supplement Series 217 (2): 27–49, doi:10.1088/0067-0049/217/2/27, Bibcode: 2015ApJS..217...27A. 
  11. ↑ Thronson, Harley A. Jr. et al. (1 August 1989), "Near-infrared image of NGC 1068 - Bar-driven star formation and the circumnuclear composition", Astrophysical Journal, Part 1 343: 158–168, doi:10.1086/167693, Bibcode: 1989ApJ...343..158T. 
  12. ↑ 12.0 12.1 12.2 Alexander, Tal; Lutz, Dieter; Sturm, Eckhard; Genzel, Reinhard; Sternberg, Amiel; Netzer, Hagai (June 2000), "Infrared Spectroscopy of NGC 1068: Probing the Obscured Ionizing AGN Continuum", The Astrophysical Journal 536 (2): 710–717, doi:10.1086/308973, Bibcode: 2000ApJ...536..710A. 
  13. ↑ de Vaucouleurs, Gérard (1973). "Southern Galaxies.VI. Luminosity Distribution in the Seyfert Galaxy NGC 1566". Astrophysical Journal 181: 31–50. doi:10.1086/152028. Bibcode: 1973ApJ...181...31D. 
  14. ↑ Wood KS; Meekins JF; Yentis DJ; Smathers HW; McNutt DP; Bleach RD (1984). "The HEAO A-1 X-ray source catalog". Astrophysical Journal Supplement Series 56 (12): 507–649. doi:10.1086/190992. Bibcode: 1984ApJS...56..507W. 
  15. ↑ King, Bob (2018-11-29). "Supernova Discovered in the Bright Galaxy M77". https://www.skyandtelescope.com/observing/supernova-discovered-in-the-bright-galaxy-m77/?k=Pg%2FjMopAjLuymaFqJZqBEJMUEcArttgJ8%2B6vHkAwjlw%3D&cid=DM88427&bid=879626371. 
  16. ↑ Observatory, European Southern (2022-02-16). "Supermassive Black Hole Caught Hiding in an Immense Ring of Cosmic Dust" (in en-US). https://scitechdaily.com/supermassive-black-hole-caught-hiding-in-an-immense-ring-of-cosmic-dust/. 
  17. ↑ IceCube Collaboration*†; Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, J. M. et al. (2022-11-04). "Evidence for neutrino emission from the nearby active galaxy NGC 1068" (in en). Science 378 (6619): 538–543. doi:10.1126/science.abg3395. ISSN 0036-8075. PMID 36378962. Bibcode: 2022Sci...378..538I. https://www.science.org/doi/10.1126/science.abg3395. 
  18. ↑ Staff. "IceCube neutrinos give us first glimpse into the inner depths of an active galaxy" (in en-US). https://icecube.wisc.edu/news/press-releases/2022/11/icecube-neutrinos-give-us-first-glimpse-into-the-inner-depths-of-an-active-galaxy/. 

External links

Coordinates: Sky map 02h 42m 40.7s, −00° 00′ 48″



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:Messier_77&oldid=3343875"