Search Publications

On the relationship between shift and intensity of ultraviolet lines in coronal holes and the quiet Sun
Bibcode: 2000A&A...362L..49S

Solanki, S. K.; Schühle, U.; Rüedi, I. +1 more

We study the relationship between wavelength shifts and intensities of chromospheric, transition-region and coronal ultraviolet emission lines in polar coronal holes and in the normal quiet Sun using SUMER data. Within coronal holes almost all the lines showing the network and formed above 30 000 K show a correlation between blueshifts and brightn…

2000 Astronomy and Astrophysics
SOHO 10
Long-term photometry of the Wolf-Rayet stars WR 137, WR 140, WR 148, and WR 153
DOI: 10.48550/arXiv.astro-ph/0002221 Bibcode: 2000A&A...355..607P

Altmann, M.; Panov, K. P.; Seggewiss, W.

In 1991, a long term UBV-photometry campaign of four Wolf-Rayet stars was started using the 60 cm telescope of the National Astronomical Observatory Rozhen, Bulgaria. Here we report on our observational results and discuss the light variations. The star WR 137 was observed during 1991 - 1998. No indications of eclipses were found, though random li…

2000 Astronomy and Astrophysics
Hipparcos 10
Clustering of galaxies at faint magnitudes
DOI: 10.48550/arXiv.astro-ph/0001105 Bibcode: 2000A&A...355...37F

Freudling, W.; Fynbo, J. U.; Möller, P.

Significant uncertainties exist in the measured amplitude of the angular two-point correlation function of galaxies at magnitudes I~26 and fainter. Published results from HST and ground-based galaxy catalogs seem to differ by as much as a factor of 3, and it is not clear whether the correlation amplitude as a function of magnitude increases or dec…

2000 Astronomy and Astrophysics
eHST 10
New infrared object in the field of the SMC cluster NGC 330
DOI: 10.48550/arXiv.astro-ph/9912090 Bibcode: 2000A&A...353L..21K

Sauvage, M.; Tanabé, T.; Vansevičius, V. +1 more

We report ISO (Infrared Space Observatory) observations of a new infrared source discovered in the vicinity of the young populous cluster NGC 330 in the Small Magellanic Cloud. The object was observed with ISOCAM at 4.5, 6.75 and 11.5 mu m and shows a prominent mid-infrared excess, indicating the presence of a dust shell. The available observation…

2000 Astronomy and Astrophysics
ISO 10
The Hipparcos, Tycho, TRC, and ACT catalogues --- A whole sky comparison of the proper motions
Bibcode: 2000A&A...360..391H

Hoogerwerf, R.; Blaauw, A.

We present a whole sky comparison of the proper motions contained in the Hipparcos Catalogue, the Tycho Catalogue, the Tycho Reference Catalogue (TRC), and the Astrographic Catalogue plus Tycho Reference Catalogue (ACT). The catalogues are compared in the 20 declination zones defined by the original Carte du Ciel project. We find that (1) the prop…

2000 Astronomy and Astrophysics
Hipparcos 10
The nature of the DAB white dwarf HS 0209+0832
Bibcode: 2000A&A...361..629W

Reimers, D.; Wolff, B.; Jordan, S. +1 more

The DAB white dwarf HS 0209+0832 is one of the few white dwarfs with detected helium in the DB gap between 28 000 and 45 000 K. We have obtained ultraviolet and optical spectra with the Hubble Space Telescope (HST). The analysis results in an effective temperature of about 35 000 K and a helium abundance of about 1%. The presenc…

2000 Astronomy and Astrophysics
eHST 10
The nearby M-dwarf system Gliese 866 revisited
DOI: 10.48550/arXiv.astro-ph/9910411 Bibcode: 2000A&A...353..253W

Franz, O. G.; Leinert, Ch.; Jahreiß, H. +3 more

We present an improved orbit determination for the visual pair in the M-dwarf triple system Gliese 866 that is based on new speckle-interferometric and HST observations. The system mass is M = 0.34+/- 0.03 Msun. The masses of the components derived using the mass-luminosity relation are consistent with this mass sum. …

2000 Astronomy and Astrophysics
eHST 10
IRAS 03201+5459: a C-rich AGB star with silicate absorption
Bibcode: 2000A&A...362..273J

Szczerba, R.; Jiang, B. W.; Deguchi, S.

IRAS 03201+5459 is a late-type star with a circumstellar envelope according to its IRAS color. It has no identification at optical or near-infrared wavelengths. A full ISO-SWS spectrum between 2.3 and 43 mu m was taken at a resolution of about ~ 300 to investigate its nature. The spectrum shows the 9.7 mu m feature in absorption, usually seen in O…

2000 Astronomy and Astrophysics
ISO 9
No QPO time lags from Sco X-1 as seen with EXOSAT: a comparison with Cyg X-2
DOI: 10.48550/arXiv.astro-ph/9911287 Bibcode: 2000A&A...353..203D

Kuulkers, Erik; van der Klis, Michiel; Lamb, Frederick K. +2 more

We have measured the phase-delay and rms amplitude spectra of Cyg X-2 and Sco X-1. Using EXOSAT data from the normal branch of Cyg X-2 we confirm earlier (Ginga) results, showing that at an energy near 6 keV there is both a minimum in the quasi-periodic oscillations QPO rms amplitude spectrum and a 150deg phase jump in the QPO phase-del…

2000 Astronomy and Astrophysics
Exosat 9
Long-duration cosmic ray modulation from a Sun-Earth L1 orbit
Bibcode: 2000A&A...362L..21P

Harrison, R. A.; Pike, C. D.

We analyse cosmic ray hits impacting the detector system of the Coronal Diagnostic Spectrometer aboard the Solar and Heliospheric Observatory spacecraft. These observations allow us to study the modulation of cosmic rays over a 4 year period (1996-2000) running from solar minimum to maximum, from a Sun-Earth L1 Lagrangian orbit. The modulation, at…

2000 Astronomy and Astrophysics
SOHO 9