Search Publications

V 439 CYG as a Late Phase of Stellar Evolution
DOI: 10.1023/A:1001186329616 Bibcode: 1998Ap&SS.255..197N

Rossi, C.; Viotti, R.; Norci, L. +2 more

1998 Astrophysics and Space Science
ISO 0
Rapid continuum variability in NGC 4151
DOI: 10.1016/S0273-1177(97)00616-9 Bibcode: 1998AdSpR..21...77E

Crenshaw, D. M.; Malkan, M.; Warwick, R. +4 more

Intensive monitoring of NGC 4151 showed strong, correlated variability at X-ray, ultraviolet, and optical wavelengths. The strongest variations were seen in ~1.5 keV X-rays, with weaker variations at ~100 keV and no significant variability in the 0.1-1 keV bands. In the ultraviolet/optical regime, the fractional variability amplitude decreased fro…

1998 Advances in Space Research
IUE 0
Obscured AGB Stars in the LMC
DOI: 10.1023/A:1001524915929 Bibcode: 1998Ap&SS.255..403V

Waters, L. B. F. M.; Whitelock, Patricia A.; Groenewegen, M. A. T. +5 more

1998 Astrophysics and Space Science
ISO 0
HI Infrared Line Formation in Early B-Type Stars
DOI: 10.1023/A:1001112214170 Bibcode: 1998Ap&SS.255..147Z

Waters, L. B. F. M.; Marlborough, J. M.; Zaal, P. A.

1998 Astrophysics and Space Science
ISO 0
Specialized detector techniques and electronics of the ERNE instrument onboard SOHO
DOI: 10.1016/S0920-5632(97)00532-X Bibcode: 1998NuPhS..61....6V

Valtonen, E.; Peltonen, J.; Eronen, T. +5 more

ERNE is designed to study the composition and energy spectra of particles encountered in interplanetary space in the energy range from 1 MeV/n to well beyond 500 MeV/n. Several innovative ideas had to be incorporated in the design of the instrument in order to fulfill the scientific requirements. Position-sensitive strip detectors are used in the …

1998 Nuclear Physics B Proceedings Supplements
SOHO 0
R Coronae Borealis Stars, Dust, and Evolution
DOI: 10.1023/A:1001534814479 Bibcode: 1998Ap&SS.255..479C

Clayton, Geoffrey C.

1998 Astrophysics and Space Science
ISO 0
The ISO Spectrum of the Cloud Core M17-North
DOI: 10.1023/A:1001102532400 Bibcode: 1998Ap&SS.255...53H

Henning, Th.; Klein, R.

1998 Astrophysics and Space Science
ISO 0
Doppler receiver for Cassini radio science experiments
DOI: 10.1016/S0032-0633(97)00137-2 Bibcode: 1998P&SS...46.1415C

Comoretto, G.

The Ka band tracking capability of the Cassini spacecraft allows for greater accuracy in most Radio Science experiments, but can be used only with the Goldstone DSN complex, i.e. for one third of the total time. A digital receiver has been designed to allow receiving the Ka band signal from a generic VLBI antenna. The receiver interfaces with the …

1998 Planetary and Space Science
Cassini 0
Far-Infrared Photometry of Circumstellar Matter Around Intermediate Mass Stars
DOI: 10.1023/A:1001150415562 Bibcode: 1998Ap&SS.255...45A

Burkert, A.; Ábrahám, P.; Henning, Th. +2 more

1998 Astrophysics and Space Science
ISO 0
ISO Observations of Freshly Synthesized Supernova Material
DOI: 10.1023/A:1001198615504 Bibcode: 1998Ap&SS.255..221L

Lagage, P. -O.

ISOCAM observations of Cassiopeia A (Cas A), the youngest supernova remnant known in our galaxy, are discussed. We show how these observations are of interest for the so-called Cas A Neon problem and how these observations have renewed the interest in supernovae as dust factories.

1998 Astrophysics and Space Science
ISO 0