Optical observations of SN 1988G

Details Optical observations of SN 1988G Optical observations of SN 1988G

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101...95r&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Jan. 1989, p. 95-100.

Astronomy and Astrophysics

Astronomy

2

Astronomical Photometry, Astronomical Spectroscopy, Galaxies, Supernovae, Visible Spectrum, Red Shift, Stellar Luminosity, Stellar Spectra

Scientific paper

Optical spectroscopy and photometry of the Type Ia supernova SN 1988G obtained shortly after dicovery are presented. The redshift of the parent galaxy is determined to be 7055 km/sec. Adopting a distance of 88 Mpc, the supernova has an absolute magnitude of M(B) = -18.8. Based on the luminosity and the characteristics displayed by the optical spectrum it is inferred that maximum light occurred within a few days of the discovery.

Affiliated with

Also associated with

No associations

Rating

Optical observations of SN 1988G does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Optical observations of SN 1988G, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical observations of SN 1988G will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828357