About site: Astronomy/Stars/Novae and Supernovae - Supernova, by HEASARC
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  About site: http://legacy.gsfc.nasa.gov/docs/snr.html

Title: Astronomy/Stars/Novae and Supernovae - Supernova, by HEASARC HEASARC: High Energy Astrophysics Science Archive Research Center provides a short article regarding the high-energy aspects of supernovae explosions.
SuperNova_Early_Warning_System_(SNEWS) Network utilizing neutrino detectors to detect neutrino burst from supernova in order to provide a prompt alert to astronomers.

Supernova_Taxonomy A discussion of the taxonomy of supernovae.

Supernovae Fundamentals of type I & II supernovae

Type_1a_Supernovae_and_the_Cosmological_Constant Brief look at recent type Ia supernova data and the cosmological constant

University_of_Texas_Supernovae_Research Includes research contacts, preprints, reviews and published papers by the Astronomy group of the University of Texas.

Very-Late-Type_Spiral_and_Irregular_Galaxy_Supernova_Search Current statistics of search at University of Iowa, movies of observed SNe. The rates in Sdm-Sm and Irr galaxies seem to be higher even than in late type Sbc-Sd galaxies.


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Supernova

animation of supernova explosionOne of the most energetic explosive events known is a supernova. These occur at the end of a star's lifetime, when its nuclear fuel is exhausted and it is no longer supported by the release of nuclear energy. If the star is particularly massive, then its core will collapse and in so doing will release a huge amount of energy. This will cause a blast wave that ejects the star's envelope into interstellar space. The result of the collapse may be, in some cases, a rapidly rotating neutron star that can be observed many years later as a radio pulsar. While many supernovae have been seen in nearby galaxies, they arerelatively rare events in our own galaxy. The last to be seen was Kepler'sstar in 1604. This remnant has been studied by many X-ray astronomy satellites,including ROSAT. There are,however, many remnants of Supernovae explosions in our galaxy, that areseen as X-ray shell likestructures caused by the shock wave propagating out into theinterstellar medium. Another famous remnant is the Crab Nebula which explodedin 1054. In this case a pulsar is seen which rotates 30 times a second andemits a rotating beam of X-rays (like a lighthouse). Another dramaticsupernova remnant is the Cygnus Loop.The set of small GIF images used to create the supernova inline animation is available.See also the X-ray binary and black hole inline animations.Visit the HEASARC Images and Video Archive. You are visitor number80753.This file was last modified on Thursday, 26-Jun-2003 13:48:43 EDTWeb page maintained bypaint pot iconPat Tylertyler@universe.gsfc.nasa.gov HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/PublicLast modified: Thursday, 26-Jun-2003 13:48:43 EDT
 

HEASARC:

High

Energy

Astrophysics

Science

Archive

Research

Center

provides

a

short

article

regarding

the

high-energy

aspects

of

supernovae

explosions.

http://legacy.gsfc.nasa.gov/docs/snr.html

Supernova, by HEASARC 2009 January

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HEASARC: High Energy Astrophysics Science Archive Research Center provides a short article regarding the high-energy aspects of supernovae explosions.

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