Search Publications

A proper motion study of the globular cluster M 10
DOI: 10.1051/aas:2000238 Bibcode: 2000A&AS..145..223C

Chen, L.; Geffert, M.; Wang, J. J. +2 more

We present the first proper motion study of M 10 (NGC 6254). Absolute proper motions of about 532 stars in the field of the globular cluster M 10 were determined with respect to Hipparcos and ACT reference stars. In addition to photographic plates of Bonn and Shanghai also wide field CCD observations as second epoch plates were used. The wide fiel…

2000 Astronomy and Astrophysics Supplement Series
Hipparcos 11
Extreme-Ultraviolet Flares in an F2 Star
DOI: 10.1086/317202 Bibcode: 2000ApJ...544..475M

Mullan, D. J.; Mathioudakis, M.

We report on the coronal properties of two early F dwarfs. For both stars, spectroscopic data reveal a hot corona with material at temperatures as high as 107.1-107.2 K. The EUV photometric observations of one of the stars (HR 120: F2) reveal two large flares with rapid decay times. The rapid decays are in striking contrast w…

2000 The Astrophysical Journal
IUE 11
Shaping of elliptical planetary nebulae. The influence of dust-driven winds of AGB stars
Bibcode: 2000A&A...354..573R

Höfner, Susanne; Reimers, Christian; Dorfi, Ernst A.

We calculated a model to investigate the shaping of a PN morphological group, i.e. elliptical PNe, in terms of the so-called Interacting Winds Model. The angle-dependent mass loss generated by a dust driven wind due to a slow rotation of the AGB star is an effective way for the shaping of PNe. The matter which is more concentrated in the equatoria…

2000 Astronomy and Astrophysics
eHST 11
The Ultraviolet Spectrum of VV Cephei Out of Eclipse
DOI: 10.1086/316479 Bibcode: 2000PASP..112...31B

Bennett, Philip D.; Bauer, Wendy Hagen

The International Ultraviolet Explorer (IUE) satellite observed VV Cephei (M2 Iab+B?) over nearly a full 20.3 year orbital period, but all the observations were obtained outside total eclipse. Egress of the chromospheric eclipse was the only portion of the eclipse observed by IUE. We have examined all 124 high-resolution IUE spectra of VV Cephei a…

2000 Publications of the Astronomical Society of the Pacific
IUE 11
The SOHO-Stellar Connection
DOI: 10.1023/A:1005200124453 Bibcode: 2000SoPh..193..273A

Ayres, Thomas R.

The `solar- stellar connection' bridges the daytime and nighttime communities; an essential link between the singular, but detailed, views of our Sun, and the broad, but coarse, glimpses of the distant stars. One area in particular - magnetic activity - has profited greatly from the two way traffic in ideas. In that spirit, I present an evolutiona…

2000 Solar Physics
SOHO eHST 11
Simulation of Nonlinear Waves in a Magnetic Flux Tube near the Quiet Solar Photospheric Network
DOI: 10.1086/317254 Bibcode: 2000ApJ...544.1108S

Sakai, J. I.; Mizuhata, Y.; Kawata, T. +1 more

Recent high-resolution observations from photospheric magnetograms made with the SOHO/Michelson Doppler Imager instrument and Swedish Vacuum Solar Telescope on La Palma showed that magnetic flux tubes in the quiet photospheric network of the solar photosphere are highly dynamic objects with small-scale substructures. We investigate nonlinear waves…

2000 The Astrophysical Journal
SOHO 11
Spectroscopic confirmation of a white dwarf companion to the B star 16 Dra
DOI: 10.48550/arXiv.astro-ph/0005426 Bibcode: 2000A&A...359..977B

Barstow, M. A.; Burleigh, M. R.

Using an Extreme Ultraviolet Explorer (EUVE) spectrum, we confirm the identification of a white dwarf companion to the B9.5V star 16 Dra (HD150100), and constrain its surface temperature to lie between 29,000 K and 35,000 K. This is the third B star + white dwarf non-interacting Sirius-type binary to be confirmed, after y Pup (HR2875, HD59635) and…

2000 Astronomy and Astrophysics
IUE 10
Vertical motions in the disk of NGC 5668 as seen with optical Fabry-Perot spectroscopy
DOI: 10.48550/arXiv.astro-ph/0004295 Bibcode: 2000A&A...358..812J

Battaner, E.; Jiménez-Vicente, J.

We have observed the nearly face-on spiral galaxy NGC 5668 with the TAURUS II Fabry-Perot interferometer at the William Herschel Telescope using the Hα line to study the kinematics of the ionized gas. From the extracted data cube we construct intensity, velocity and velocity dispersion maps. We calculate the rotation curve in the innermost 2 arcmi…

2000 Astronomy and Astrophysics
eHST 10
CaII K Emission-Line Asymmetry among Red Giants Detected by the ROSAT Satellite
DOI: 10.1086/316634 Bibcode: 2000PASP..112.1320S

Smith, Graeme H.; Shetrone, Matthew D.

Spectra of the Ca II H and K lines are reported for a number of field giants from which soft X-ray emission was detected by the ROSAT satellite. Several of these stars are RS CVn systems and exhibit very strong Ca II emission. The majority of the noninteracting giants in the sample have MV>-2.0, as determined from Hipparcos parallaxe…

2000 Publications of the Astronomical Society of the Pacific
Hipparcos 10
Kinematics and morphology of the narrow-line region in the Seyfert galaxy NGC 1386
DOI: 10.48550/arXiv.astro-ph/0008269 Bibcode: 2000A&A...362..501R

Dietrich, M.; Wagner, S. J.; Rossa, J.

We present a high spatial and spectral resolution 2-D echelle spectrogram of the Narrow-Line Region in the Seyfert 2 galaxy NGC 1386. This Seyfert galaxy was observed with CASPEC in the wavelength range 5270-7725 Å which covers the Hα and the [N Ii] lines. With the use of spatially high resolved images taken with the WFPC2 aboar…

2000 Astronomy and Astrophysics
eHST 10