Published February 1987
| Version v1
Journal article
CCD photometry of E1013-477 - an intermediate polar system?
Description
The first I-band CCD photometry of the AM Her candidate E1013-477 in a faint state has been obtained. There is no evidence for any periodicity near the claimed 103.4 min orbital period; however, significant variability on a time scale of about 6.4 hrs and a possible period of 71.1 min are observed. It is proposed that E1013-477 may be an intermediate polar system. This interpretation is also consistent with previous observations. 21 references
Additional details
Publishing Information
- Journal Title
- Publ. Astron. Soc. Pac.
- Journal Volume
- 99
- Series
- Publ. Astron. Soc. Pac.
- Journal Page Range
- 149-153
- ISSN
- 0004-6280
- CODEN
- PASPA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18097049
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; COSMIC X-RAY SOURCES; ERUPTIVE VARIABLE STARS; PHOTOMETRY; WHITE DWARF STARS
- Descriptors DEC
- COSMIC RAY SOURCES; DWARF STARS; STARS; VARIABLE STARS