Great Annihilator

This article is about the astronomical object. For the Swans album, see The Great Annihilator.
Great Annihilator
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 17h 43m 54.83s[1]
Declination −29° 44′ 42.6″[1]
Astrometry
Distance16,000 ly
(5,000[2] pc)
Database references
SIMBADdata

1E1740.7-2942, or the Great Annihilator,[3][4] is a Milky Way microquasar, located near the Galactic Center on the sky.[5][2] It likely consists of a black hole and a companion star. It is one of the brightest X-ray sources in the region around the Galactic Center.[6]

The object was first detected in soft X-rays by the Einstein Observatory,[7] and later detected in hard X-rays by the Soviet Granat space observatory.[2] Followup observations by the SIGMA detector on board Granat showed that the object was a variable emitter of massive amounts of photon pairs at 511 keV, which usually indicates the annihilation of an electron-positron pair.[8][9] This led to the nickname, "Great Annihilator."[10] Early observations also showed a spectrum similar to that of the Cygnus X-l, a black hole with a stellar companion, which suggested that Great Annihilator was also a stellar mass black hole.[8]

The object also has a radio source counterpart that emits jets approximately 1.5 pc (5 ly) long.[11] These jets are probably synchrotron emission from positron-electron pairs streaming out at high velocities from the source of antimatter. Modeling of the observed precession of these jets gives an object distance of approximately 5 kpc (or 16,000 ly).[2] This means that while the object is likely located along our line of sight towards the center of the Milky Way, it may be closer to us than Sagittarius A*, the black hole at the center of our galaxy.

  1. ^ a b "NAME Great Annihilator". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ a b c d Luque-Escamilla, Pedro L.; Martí, Josep; Martínez-Aroza, José (2015-12-01). "The precessing jets of 1E 1740.7−2942". Astronomy & Astrophysics. 584: A122. arXiv:1511.01425. doi:10.1051/0004-6361/201527238. ISSN 0004-6361.
  3. ^ Sunyaev, R. A.; Borozdin, K. N.; Aleksandrovich, N. L.; Arefev, V. A.; Kaniovskii, A. S.; Efremov, V. V.; Maisack, M.; Reppin, C.; Skinner, J. K. (November 1994). "Observations of X-ray novae in Vela (1993), Ophiuchus (1993), and Perseus (1992) using the instruments of the Mir-Kvant module". Astronomy Letters. 20 (6): 777. Bibcode:1994AstL...20..777S.
  4. ^ Odenwald, Sten (1997). "What do we know about the 'Great Annihilator' in the center of the Milky Way?". Astronomy Cafe. Archived from the original on 16 January 2013. Retrieved 4 August 2014.
  5. ^ Mirabel, I. F. "The Great Annihilator in the Central Region of the Galaxy" (PDF). eso.org. pp. 51–54.
  6. ^ Stecchini, Paulo Eduardo; Castro, Manuel; Jablonski, Francisco; D’Amico, Flavio; Braga, João (2017-06-30). "Tandem Swift and INTEGRAL Data to Revisit the Orbital and Superorbital Periods of 1E 1740.7–2942". The Astrophysical Journal. 843 (1): L10. arXiv:1707.00730. Bibcode:2017ApJ...843L..10S. doi:10.3847/2041-8213/aa7942. ISSN 2041-8213. S2CID 119354178.
  7. ^ Hertz, P.; Grindlay, J. E. (1984-03-01). "The Einstein galactic plane survey : statistical analysis of the complete X-ray sample". The Astrophysical Journal. 278: 137–149. Bibcode:1984ApJ...278..137H. doi:10.1086/161775. ISSN 0004-637X.
  8. ^ a b Sunyaev, R.; Churazov, E.; Gilfanov, M.; Pavlinsky, M.; Grebenev, S.; Babalyan, G.; Dekhanov, I.; Khavenson, N.; Bouchet, L.; Mandrou, P.; Roques, J. P. (December 1991). "Three spectral states of 1E 1740.7-2942 – From standard Cygnus X-1 type spectrum to the evidence of electron-positron annihilation feature". The Astrophysical Journal. 383: L49. Bibcode:1991ApJ...383L..49S. doi:10.1086/186238. ISSN 0004-637X.
  9. ^ Bouchet, L.; Mandrou, P.; Roques, J. P.; Vedrenne, G.; Cordier, B.; Goldwurm, A.; Lebrun, F.; Paul, J.; Sunyaev, R.; Churazov, E.; Gilfanov, M. (December 1991). "Sigma discovery of variable e(+)–e(−) annihilation radiation from the near Galactic center variable compact source 1E 1740.7-2942". The Astrophysical Journal. 383: L45. Bibcode:1991ApJ...383L..45B. doi:10.1086/186237. ISSN 0004-637X.
  10. ^ "Milky Way Monster". Time. 1992-07-27. ISSN 0040-781X. Retrieved 2019-10-24.
  11. ^ Mirabel, I. F.; Rodríguez, L. F.; Cordier, B.; Paul, J.; Lebrun, F. (July 1992). "A double-sided radio jet from the compact Galactic Centre annihilator 1E1740.7–2942". Nature. 358 (6383): 215–217. Bibcode:1992Natur.358..215M. doi:10.1038/358215a0. ISSN 0028-0836. S2CID 4264588.