Published October 1, 1990
| Version v1
Journal article
Infrared photometry and spectroscopy of nova PW Vul 1984
- 1. Keele Univ. (UK). Dept. of Physics
- 2. Anglo-Australian Observatory, Epping (Australia)
- 3. South African Astronomical Observatory, Cape Town (South Africa)
Description
We present near-infrared photometry and spectroscopy of the slow nova PW Vul (Nova Vul 1984 No. 1) prior to its dust-formation phase. In common with the visual light curve, the near-infrared light curves varied extremely erratically during the first 100 d after maximum. Emission lines of C and N were prominent in the near-infrared spectra, as would be expected from the thermonuclear-runaway model of the nova outburst, but He I lines were weak. A distance of 3 kpc is consistent with a number of independent distance indicators. (author)
Additional details
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 246
- Journal Issue
- 3
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 527-534
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 22067707
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- COLOR; DISTANCE; EXPERIMENTAL DATA; NEAR INFRARED RADIATION; NOVAE; PHOTOMETRY; SPECTROSCOPY; VISIBLE RADIATION
- Descriptors DEC
- BINARY STARS; DATA; ELECTROMAGNETIC RADIATION; ERUPTIVE VARIABLE STARS; INFORMATION; INFRARED RADIATION; NUMERICAL DATA; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS; VARIABLE STARS