Search Publications

An analysis of the Ap binary HD 81009
Bibcode: 2000A&A...361..991W

Wade, G. A.; Bohlender, D. A.; Mathys, G. +3 more

We present a detailed investigation of the orbit, component characteristics and magnetic field of the single spectrum (SB1), visual Ap binary HD 81009. By simultaneously modeling new and archival radial velocity measurements and new and archival speckle interferometric measurements (obtained with the CHARA array) we obtain a unique model of the or…

2000 Astronomy and Astrophysics
Hipparcos 12
Orbital period variation in close binaries from radial velocity data and magnetic activity cycles. I. AR Lacertae: The test case
Bibcode: 2000A&A...356..267F

Lanza, A. F.; Frasca, A.

We check the possibility of detecting orbital period changes in non-eclipsing close binaries by means of spectroscopic orbit determinations. In order to test our method, we selected the eclipsing binary AR Lacertae for which the spectroscopically determined epochs of superior conjuctions can be compared with those provided by the light minima phot…

2000 Astronomy and Astrophysics
IUE 12
The bright 175 mu m knots of the Andromeda galaxy
DOI: 10.48550/arXiv.astro-ph/0009494 Bibcode: 2000A&A...363..917S

Lemke, D.; Haas, M.; Schmidtobreick, L.

Discrete far-infrared (FIR) sources of M 31 are identified in the ISO 175 mu m map and characterized via their FIR colours, luminosities and masses in order to reveal the nature of these knots. With our spatial resolution of 300 pc at M 31's distance, the FIR knots are clearly seen as extended objects with a mean size of about 800 pc. Since this a…

2000 Astronomy and Astrophysics
ISO 12
Decaying post-flare loops system observed by SOHO/CDS and Yohkoh/SXT
Bibcode: 2000A&A...355..769V

Heinzel, P.; Fludra, A.; Varady, M.

The results of an analysis of joint SOHO/CDS and Yohkoh/SXT observations of a decaying post-flare loops system with a rapid time evolution are presented. The loop system was a remnant of a small single loop flare (GOES class C2.9). Using the CDS raster taken in several EUV lines with different formation temperatures and a temperature sensitive lin…

2000 Astronomy and Astrophysics
SOHO 11
ORFEUS II echelle spectra: on the influence of iron-group line blanketing in the Far-UV spectral range of hot subdwarfs
DOI: 10.48550/arXiv.astro-ph/0006341 Bibcode: 2000A&A...360..281D

Deetjen, J. L.

We present an analysis of the subdwarf O star Feige 67 with a fully metal-line blanketed NLTE model atmosphere based on high-resolution Far-UV (912-2000 Å) and Near-UV (2000-3400 Å) spectra from new ORFEUS II echelle observations and the IUE final archive. The Far- UV spectra are heavily blanketed by iron and nickel lines, preventing the detection…

2000 Astronomy and Astrophysics
IUE 11
Solar equatorial plasma rotation: a comparison of different spectroscopic measurements
Bibcode: 2000A&A...357..763W

Schmidt, W.; Wöhl, H.

We present solar equatorial rotation velocities measured with two different spectral lines (Fe I 557.6 nm and Ni I 676.8 nm) and two different spectrometers at the German Vacuum Tower Telescope (VTT) on Tenerife. The `classical' sidereal solar equatorial rotation velocity of about 2000 m/s has been confirmed. The results are compared with those fr…

2000 Astronomy and Astrophysics
SOHO 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
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
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