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ASASSN-15lh

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This is an old revision of this page, as edited by 106.69.51.23 (talk) at 00:57, 18 January 2016 (3 orders of mag = 2.512^3 =15.8. Let's call it ~15 since there is there is error of ± 0.1 in abs mag). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

ASASSN-15lh
Hypernova
ConstellationIndus
Right ascension22h 2m 15.45s[1]
Declination−61° 39′ 34.64″[1]
EpochJ2000
Distance3.8 billion light years
Redshift0.2326 Edit this on Wikidata
[edit on Wikidata]

ASASSN-15lh is a superluminous supernova that was detected by the All Sky Automated Survey for SuperNovae (ASAS-SN) in 2015 in the southern constellation Indus.[1] The discovery, confirmed by ASAS-SN group with several other telescopes,[1] was formally described and published on January 15, 2016. ASASSN-15lh is the most luminous supernova ever detected; at its brightest it was approximately 15 times more luminous than the entire Milky Way,[2] with an energy hundreds of billions times greater than the Sun.[3] The peak absolute magnitude was −23.5, putting out 2×1047 ergs per second. Energy radiated exceeded 1052 ergs. The supernova was at redshift 0.2326, in a stagnant but luminous galaxy[4] some 3.8 billion light years from Earth.[3] According to Krzysztof Stanek of Ohio State University, one of the principal investigators at ASAS-SN, "If it was in our own galaxy, it would shine brighter than the full moon; there would be no night, and it would be easily seen during the day."[5]

Discovery

ASASSN-15lh was first observed in June 2015 by ASAS-SN’s twin 14-cm telescopes in Chile.[6] The supernova appeared as a transient dot of light on an image and confirmed with additional observations from other telescopes.[6] The observations detected the outburst’s fading afterglow, while the spectrum of ASASSN-15lh was provided by the 2.5-meter du Pont Telescope in Chile.[6] Swift space telescope and large telescopes in South Africa also joined the observations. At its peak, ASASSN-15lh was twice as luminous as the previous brightest superluminous supernova, iPTF13ajg.[7]

Previously observed superluminous supernovae (known as SLSNe) have been discovered in relatively small and "busy" star-producing galaxies, in contrast to ASASSN-15lh, which lies in a large and relatively calm galaxy of a type not previously known for producing superluminous supernovae.[8] Such explosions are 100 to 1,000 times as powerful as typical supernovae.

Suggested mechanisms

The precise mechanism underlying the very large ASASSN-15lh explosion is still unknown, with speculation ranging from the presence of very large quantities of decaying nickel to the amplifying effects of a magnetar. Its unusual location in a relatively quiescent galaxy may offer clues for scientists to discover and observe similar events.[8] The constraints are such that the magnetar model has been described as "just barely" able to explain the data,[6] but is nevertheless still thought to be "the most plausible explanation for ASASSN-15lh’s unprecedented brightness".[9] If instead it was caused by the death of a huge star astronomers should eventually be able to detect the "fading afterglow caused by the gradual decay of 30 solar masses’ worth of radioactive nickel";[6] the data indicate that the supernova was hydrogen-poor,[6][1] and previously observed hydrogen-poor superluminous supernovae explosions cannot be fully explained by their radioactive nickel-56.[1] Observations by the Hubble Space Telescope scheduled for February 2016 may give rise to another scenario, albeit one thought to be unlikely, that the supernova is in the nucleus of its galaxy and that its brightness is due to its interaction with a supermassive black hole there.[9]

Progenitor

ASASSN-15lh emitted a blue-colored light towards Earth.[1] The progenitor of ASASSN-15lh may have been a massive and rapidly-rotating blue, hot star,[9] which appears to have shed its surface layers of hydrogen and helium not long before its explosion as those elements are absent in ASASSN-15lh.[9] It may have been a Wolf–Rayet star.[9]

References

  1. ^ a b c d e f g Young, Monica (July 12, 2015). "The Most Luminous Supernova". Sky & Telescope. Retrieved January 16, 2016.
  2. ^ Carnegie Institution for Science (January 14, 2016). "Most-luminous supernova ever discovered". phys.org. Retrieved January 15, 2016.
  3. ^ a b Bhanoo, Sindya N. (January 15, 2016). "Supernova Has Energy of Hundreds of Billions of Suns". The New York Times. Retrieved January 16, 2016.
  4. ^ Dong, S.; Shappee, B. J.; Prieto, J. L.; Jha, S. W.; Stanek, K. Z.; Holoien, T. W.- S.; Kochanek, C. S.; Thompson, T. A.; Morrell, N.; Thompson, I. B.; et al. (January 14, 2016). "ASASSN-15lh: A highly super-luminous supernova". Science. 351 (6270): 257–260. arXiv:1507.03010. doi:10.1126/science.aac9613.
  5. ^ Boyle, Rebecca (January 14, 2016). "We've found the brightest ever supernova but can't explain it". New Scientist. Retrieved January 15, 2016.
  6. ^ a b c d e f Billings, Lee (January 14, 2016). "Found: The Most Powerful Supernova Ever Seen". Scientific American. Retrieved January 16, 2016.
  7. ^ Young, Monica (January 15, 2016). "Brightest Supernova Baffles Astronomers". Sky & Telescope. Retrieved January 16, 2016.
  8. ^ a b Thomson, Jason (January 14, 2016). "Astronomers spot brightest supernova in history". The Christian Science Monitor. Retrieved January 15, 2016.
  9. ^ a b c d e Smith-Strickland, Kiona (January 14, 2016). "Brightest supernova ever seen pushes theoretical models to the edge". Astronomy. Retrieved January 17, 2016.

Further reading

Retrieved from "https://en.wikipedia.org/w/index.php?title=ASASSN-15lh&oldid=700356499"