SN 1998S

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

  1. REDIRECT Template:Infobox astronomical event

SN 1998S was a type IIn supernova that was detected in NGC 3877 in March 1998. At the time of discovery, SN 1998S was the brightest type IIn event observed,[1] although later outshone by SN 2010jl.[2]

It was discovered on 1998 March 2.68 UT in NGC 3877 by Z. Wan at a broadband (unfiltered) optical magnitude of +15.2.

Its spectrum showed prominent H and He emission lines with narrow peaks and broad wings, superimposed on a blue continuum. These narrow lines indicate the presence of a dense circumstellar medium (CSM) in the vicinity of the supernova. The high luminosity of SN1998S is due to the interaction of fast material (ejecta) with previously-expelled slowly-expanding material (CSM), which can more effectively convert kinetic energy of ejecta into radiation energy.[3]

References

<templatestyles src="Reflist/styles.css" />

  1. Script error: No such module "Citation/CS1".
  2. Script error: No such module "Citation/CS1".
  3. Script error: No such module "Citation/CS1".

Script error: No such module "Check for unknown parameters".

External links


Template:Asbox