-
higher than most supernovae, with a
luminosity at
least 10
times greater.
Hypernovae release such
intense gamma rays that they
often appear similar to a type...
- than the norm. The most
luminous type Ic
supernovae are
referred to as
hypernovae and tend to have
broadened light curves in
addition to the
increased peak...
-
Photodisintegration (also
called phototran****ation, or a
photonuclear reaction) is a
nuclear process in
which an
atomic nucleus absorbs a high-energy...
- candidates. Long
duration GRBs are
related to
superluminous supernovae, or
hypernovae, and most
luminous blue
variables (LBVs) and
rapidly spinning Wolf–Rayet...
-
Mazzali PA,
Nomoto K,
Lazzati D,
Cappellaro E (2004). "The
Rates of
Hypernovae and Gamma-Ray Bursts:
Implications for
Their Progenitors". Astrophysical...
- Thielemann, Friedrich-Karl (10 July 2001). "Explosive
Nucleosynthesis in
Hypernovae". The
Astrophysical Journal. 555 (2): 880–899. arXiv:astro-ph/0011184...
- of a
black hole born from an
extremely m****ive star,
others including hypernovae and long-duration gamma-ray bursts. Theoretically, a red
supergiant star...
- arXiv:astro-ph/0407451. Bibcode:2004ESASP.552..185V. Pair
Instability Supernovae and
Hypernovae.,
Nicolay J. Hammer, (2003),
accessed May 7, 2007.
Archived June 8, 2012...
- hypernova. They have been
observed to last 90 to 200 seconds.
Nearly all
hypernovae are
detected via (higher-energy) gamma-ray photons, at
distances too great...
- PS1-10adi is an
unusual and
highly energetic optical transient discovered by the Pan-STARRS
survey on 15
August 2010. The
explosion or
transient event...
