Ultraviolet properties of the symbiotic stars
1982 ◽
Vol 70
◽
pp. 103-113
Prior to the launch of the IDE satellite in early 1978, the only symbiotic star previously detected in the ultraviolet by earlier UV satellites, such as the 0A0-2, TD-1 and ANS experiments, was AG Pegasi = HD 207757 (Gallager et al. 1979). These broad-band observations indicated that the symbiotics as a class may show a significant ultraviolet flux and thus they became natural candidates for a survey with the IUE satellite. The following is an interim report on a survey of the symbiotics, both at low and, for AG Pegasi and CH Cygni, at high resolution.
2006 ◽
Vol 2
(14)
◽
pp. 169-194
Keyword(s):
2017 ◽
Vol 14
(S339)
◽
pp. 291-294
Keyword(s):
1990 ◽
Vol 122
◽
pp. 444-445
1990 ◽
Vol 122
◽
pp. 440-441
Keyword(s):
1982 ◽
Vol 70
◽
pp. 269-272
2004 ◽
Vol 215
◽
pp. 168-169
◽
Keyword(s):
1982 ◽
Vol 70
◽
pp. 131-136
Keyword(s):