Abstract
CPD - 26/sup 0/389, a hot subdwarf at the centre of the planetary nebula NGC 1360, is shown to be a single-lined spectroscopic binary with a period of about 8 day. The primary (visible) component appears to be less massive than its companion, and the total stellar mass of the system is presumably below one solar mass.
Mendez, R H;
Niemela, V S
[1]
- Instituto de Astronomia y Fisica del Espacio, Buenos Aires (Argentina)
Citation Formats
Mendez, R H, and Niemela, V S.
Central star of NGC 1360: a spectroscopic binary within a planetary nebula.
United Kingdom: N. p.,
1977.
Web.
Mendez, R H, & Niemela, V S.
Central star of NGC 1360: a spectroscopic binary within a planetary nebula.
United Kingdom.
Mendez, R H, and Niemela, V S.
1977.
"Central star of NGC 1360: a spectroscopic binary within a planetary nebula."
United Kingdom.
@misc{etde_7223035,
title = {Central star of NGC 1360: a spectroscopic binary within a planetary nebula}
author = {Mendez, R H, and Niemela, V S}
abstractNote = {CPD - 26/sup 0/389, a hot subdwarf at the centre of the planetary nebula NGC 1360, is shown to be a single-lined spectroscopic binary with a period of about 8 day. The primary (visible) component appears to be less massive than its companion, and the total stellar mass of the system is presumably below one solar mass.}
journal = []
volume = {178:2}
journal type = {AC}
place = {United Kingdom}
year = {1977}
month = {Feb}
}
title = {Central star of NGC 1360: a spectroscopic binary within a planetary nebula}
author = {Mendez, R H, and Niemela, V S}
abstractNote = {CPD - 26/sup 0/389, a hot subdwarf at the centre of the planetary nebula NGC 1360, is shown to be a single-lined spectroscopic binary with a period of about 8 day. The primary (visible) component appears to be less massive than its companion, and the total stellar mass of the system is presumably below one solar mass.}
journal = []
volume = {178:2}
journal type = {AC}
place = {United Kingdom}
year = {1977}
month = {Feb}
}