Published December 1979
| Version v1
Journal article
Spectrum of supernova 1972e in NGC 5253
Creators
- 1. Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma 73019
Description
Photoelectric scans of the spectrum of SN 1972e are presented. The observations were obtained at the McDonald Observatory between 15 and 50 days after maximum light with a spectral resolution ranging from 4 to 20 Angstroms. Line identifications (Ca II, Fe II, Si II, and possibly He I) are discussed briefly. It is suggested that the emission feature identified by Kirshner and Oke as Hα may have been produced by Fe II
Additional details
Publishing Information
- Journal Title
- Astron. J.
- Journal Volume
- 84
- Journal Issue
- 12
- Series
- Astron. J.
- Journal Page Range
- 1837-1839
- ISSN
- 0004-6256
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 11519502
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; CALCIUM IONS; EMISSION SPECTRA; GALAXIES; HELIUM; IRON IONS; PHOTOMETRY; SILICON IONS; SUPERNOVAE
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; ELEMENTS; ERUPTIVE VARIABLE STARS; IONS; NONMETALS; RARE GASES; SPECTRA; STARS; VARIABLE STARS