Published March 1976
| Version v1
Journal article
Interstellar lines in the spectrum of Nova Cygni 1975
Description
It is found that in the spectrum of Nova Cygni 1975 the interstellar line consists of three components. The radial velocity of the strongest component is -11.0 kms-1, and the equivalent width of interstellar Ca II K line measured for this component amounts to 192 mA. This value of equivalent width indicates that the distance modulus of the nova is msub(v) - Msub(v) = 10.9 +- 1.3 mag. (auth.)
Additional details
Identifiers
Publishing Information
- Journal Title
- Publications of the Astronomical Society of Japan
- Journal Volume
- 28
- Journal Issue
- 1
- Series
- Publ. Astron. Soc. Jpn.
- Journal Page Range
- 171-174
- ISSN
- 2053-051X
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 8294479
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION SPECTRA; CALCIUM IONS; COSMIC GASES; DISTANCE; EMISSION SPECTRA; NOVAE; RADIAL VELOCITY; SPECTROPHOTOMETRY; VISIBLE RADIATION
- Descriptors DEC
- ATOMIC IONS; CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; FLUIDS; GASES; IONS; RADIATIONS; SPECTRA; STARS; VELOCITY
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent