The photopolarimeter on ISO (ISOPHOT) has been used to investigate the dust discs around the four prototype Vega-like stars and several main sequence stars with excess infrared emission from IRAS data.
Infrared Mapping of the Dust Around Main Sequence Stars
1998-12-01
Conference paper
No indication
English
Infrared Mapping of The Dust Around Main Sequence Stars
NTRS | 1998
|Dust Around Main Sequence and Evolved Stars
British Library Conference Proceedings | 1998
|Dust Around Main Sequence and Evolved Stars
Online Contents | 1998
|Understanding the main-sequence stars.
NTRS | 1963
|Modelling the dust around Vega-like stars
British Library Conference Proceedings | 1996
|