APM 08279+5255
| APM 08279+5255 | |
|---|---|
| Observation data (Epoch 2011) | |
| Constellation | Lynx |
| Right ascension | 08h 31m 41.60s |
| Declination | 52° 45′ 16.8″ |
| Distance | 12×109 LY |
| See also: Quasar, List of quasars | |
|
|
This article needs attention from an expert on the subject. See the talk page for details. WikiProject Science or the Science Portal may be able to help recruit an expert. (November 2008) |
APM 08279+5255 is a quasar in the constellation Lynx,[1] that is notable for being a particularly good example of a gravitational lens. When originally discovered, the combination of its high redshift and brightness (particularly in the infrared) made it the most luminous object known- the light left the quasar more than 12 billion years ago (it is 12 billion light-years from Earth). High-resolution observations with the NICMOS camera on-board the Hubble Space Telescope revealed that the source was actually composed of three discrete components, with a maximum separation of 0.4 arcsec. Subsequent observations with the STIS spectrograph (also aboard HST) showed that each component has the same spectral energy distribution and therefore that each is probably an image of a single quasar. The lensing hypothesis greatly reduces the intrinsic luminosity of the lensed quasar as the observed brightness is enhanced by the magnification effect of the lens. Gravitational lens systems with odd numbers of images are extremely rare, most containing two or four.
In 2011 it was reported that vast amounts of water vapor in a cloud-like phenomenon are around this quasar, the oldest and largest mass of water in the known universe- 140 trillion times more water than that held in all of Earth's oceans combined. Its discovery shows that water has been prevalent in the known universe for nearly its entire existence- to 1.6 billion years after the Big Bang, 1 billion years earlier than any previous discovery.[2][3]
[edit] References
- ^ http://chandra.harvard.edu/photo/2003/apm08279/
- ^ Bradford; Bolatto; Maloney; Aguirre; Bock; Glenn; Kamenetzky; Lupu et al (2011). "The Water Vapor Spectrum of APM 08279+5255: X-Ray Heating and Infrared Pumping over Hundreds of Parsecs". arXiv:1106.4301 [astro-ph.CO].
- ^ "APM 08279+5255 - The Largest Water Mass In The Universe (So Far)". Science 2.0. July 22, 2011. http://www.science20.com/news_articles/apm_082795255_largest_water_mass_universe_so_far-81124.
[edit] Further reading
- Irwin, Michael J.; Ibata, Rodrigo A.; Lewis, Geraint F.; Totten, Edward J. (1998). "APM 08279+5255: An Ultraluminous Broad Absorption Line Quasar at a Redshift z = 3.87". Astrophysical Journal 505 (2): 529–535. arXiv:astro-ph/9806171. Bibcode 1998ApJ...505..529I. doi:10.1086/306213.
- Riechers, Dominik A.; Walter, Fabian; Carilli, Christopher L.; Lewis, Geraint F. (2009). "Imaging The Molecular Gas in a z = 3.9 Quasar Host Galaxy at 03 Resolution: A Central, Sub-Kiloparsec Scale Star Formation Reservoir in APM 08279+5255". Astrophysical Journal 690 (1): 463–485. Bibcode 2009ApJ...690..463R. doi:10.1088/0004-637X/690/1/463.
[edit] External links
- Article from the University of Victoria newspaper
- Detailed CCD image of APM 08279+5255 based on 60 min total exposure
- Astronomy Picture of the Day
- Chandra X-ray Observatory
- Wikisky image of APM 08279+5255
Coordinates:
08h 31m 41.60s, +52° 45′ 16.8″
| This quasar-related article is a stub. You can help Wikipedia by expanding it. |
| Wikimedia Commons has media related to: Quasars |