Published November 15, 1990 | Version v1
Journal article Metadata-only

IRAS 07027 - 7934: a probable new [WC11] star

Creators

  • 1. South African Astronomical Observatory, Cape Town (South Africa)
  • 2. Royal Observatory, Edinburgh (UK)

Description

The IRAS source 07027-7934 has been found to have a nebular spectrum together with emission lines of C II and C III superimposed on a weak continuum. The infrared and optical characteristics closely resemble those of He2-113 and CPD-5608032 which are classified as [WC11] objects, i.e., a planetary nebula with a very cool Wolf-Rayet central star. (author)

Additional details

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
247
Journal Issue
2
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
177-181
ISSN
0035-8711
CODEN
MNRAA

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
22024684
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
BALMER LINES; CARBON IONS; EXPERIMENTAL DATA; INFRARED RADIATION; LINE WIDTHS; NEBULAE; PLANETARY NEBULAE; RADIAL VELOCITY; RADIATION FLUX; STARS; VISIBLE SPECTRA; WOLF-RAYET STARS
Descriptors DEC
ATOMIC IONS; CHARGED PARTICLES; DATA; ELECTROMAGNETIC RADIATION; INFORMATION; IONS; MAIN SEQUENCE STARS; NUMERICAL DATA; RADIATIONS; SPECTRA; VELOCITY