Published December 15, 1987
| Version v1
Journal article
Orbital elements of the exnova CP Puppis
- 1. Muenster Univ. (Germany, F.R.). Astronomisches Inst.
Description
Radial velocity measurements of the exnova CP Pup yield an orbital amplitude of 92 km s-1 and a period of 0.061 4215 day, which is shorter than the photometric periods determined by a previous author. The mass of the secondary is 0.14 M of the solar mass, that of the primary is below 0.86 M of the solar mass, perhaps as low as 0.12 M of the solar mass. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 229
- Journal Issue
- 4
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 653-657
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 19048359
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- BALMER LINES; BINARY STARS; EXPERIMENTAL DATA; MASS; NOVAE; ORBITS; RADIAL VELOCITY; VARIATIONS; VISIBLE SPECTRA
- Descriptors DEC
- DATA; ERUPTIVE VARIABLE STARS; INFORMATION; NUMERICAL DATA; SPECTRA; STARS; VARIABLE STARS; VELOCITY