Astronomy:LMC N49
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| Supernova remnant | |
|---|---|
| Observation data: J2000.0[1] epoch | |
| Right ascension | 05h 26m 01.00s[1] |
| Declination | −66° 05′ 06.0″[1] |
| Distance | 160,000[2] ly |
| Apparent magnitude (V) | 12.71[1] |
| Constellation | Dorado |
| Physical characteristics | |
| Dimensions | 75 ly across[2] |
| Designations | LMC N49,[3][1] PKS 0525-66,[3][1] PKS B0525-661,[3][1] PKS J0525-6604,[3][1] SNR J052559-660453[3][1] |
N49 or LMC N49[3] (PKS 0525-66,[1][3] PKS B0525-661,[3] PKS J0525-6604,[3] SNR J052559-660453[1]), also known as Brasil Nebula,[4] is a supernova remnant in the Large Magellanic Cloud.[2]
After a massive detection of Gamma-ray and X-ray emissions from the LMC N49 were detected on March 5, 1979 by the Venera 11, 12, other 7 spacecraft,[5] and confirmed to be particularly strong by the first X-ray telescope, the Einstein Observatory.[6] The N49 supernova remnant is also known as the Brasil Nebula, due to its shape resembling the outline of Brazil in some images.
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 "SNR J052559-660453". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=SNR+J052559-660453.
- ↑ 2.0 2.1 2.2 Chandra X-ray Observatory (2010-05-24). "N49: Stellar Shrapnel Seen in Aftermath of Explosion". http://chandra.harvard.edu/photo/2010/n49/. Retrieved 2015-10-15.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 "PKS 0525-66". NASA/IPAC Extragalactic Encyclopedia. http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=LMC+N49&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.
- ↑ Sky & Telescope, August 2004, page 12
- ↑ Cosmos, Carl Sagan, page 300
- ↑ "The Einstein Observatory (HEAO-2)" https://heasarc.gsfc.nasa.gov/docs/einstein/heao2.html
- Harvard-Smithsonian Center for Astrophysics, "N49: A supernova remnant in the Large Magellanic Cloud"
