Search Publications

Circumstellar Absorption and Emission in the Post-AGB Stars HR4049 and HD213985
DOI: 10.1007/BF00667871 Bibcode: 1995Ap&SS.224..357W

Waters, L. B. F. M.; Van Winckel, H.; Waelkens, C. +1 more

The evolved C-rich low-mass stars HR 4049 and HD 213985 present variable circumstellar extinction and emission. Observations of HR 4049 strengthen the link between the far-UV extinction rise and the presence of small C-rich particles. Variability of the UV absorption bump in HD 213985 is reported here for the first time and is discussed.

1995 Astrophysics and Space Science
IUE 14
New kinematic distances of NGC 7009 and BD+30°3639 from UV and radio data
DOI: 10.1007/BF00626867 Bibcode: 1995Ap&SS.229..203M

Maciel, W. J.

Measurements of the equivalent width of the interstellar Lymanα line from IUE spectra in the direction of the planetary nebulae NGC 7009 and BD+30°3639 are used to infer the H column density in these directions. Hydrogen 21 cm profiles are also used in connection with the ultraviolet data so that the expected rotation velocities and distances can …

1995 Astrophysics and Space Science
IUE 12
Astronomical Archives and Their Importance for Knowledge Transfer in Basic Space Science
DOI: 10.1007/BF00984992 Bibcode: 1995Ap&SS.228..385W

Wamsteker, W.; Griffin, R. E. M.

We summarize the nature of modern astronomical archives with special reference to spectroscopic data archives and illustrate in which ways archives can play a role in the accelerated development of Basic Space Sciences in the developing countries. Some of the conflicting issues in the current planning of archives are addressed. Astronomical spectr…

1995 Astrophysics and Space Science
IUE 7
A search for planetary system candidates: Northern Nearby A Stars With Dust Disks And Circumstellar Gas
DOI: 10.1007/BF00667937 Bibcode: 1995Ap&SS.224..525N

Cheng, Kwang-Ping; Neff, James E.

We report on our search for possible planetary system candidates in a volume-limited sample of 62 nearby A stars. Since the evolutionary lifetimes of A stars (≤ 109 yrs) roughly correspond to the era of planet formation and subsequent "heavy bombardment" in our solar system, our study could provide valuable insight into the origin of ou…

1995 Astrophysics and Space Science
IUE 1