Search Publications

On the Low-Mass End of the Globular Cluster Luminosity Function
DOI: 10.1086/344498 Bibcode: 2002ApJ...578L..51S

Smith, Graeme H.; Burkert, Andreas

The low-mass globular cluster luminosity function (GCLF) in the Milky Way and in two elliptical galaxies is investigated. We find that the power-law slope of the Milky Way GCLF depends on the cluster concentration c. The origin of this trend is explored within the framework of a GC mass-loss model. It is also found that the low-mass GCLF of the Mi…

2002 The Astrophysical Journal
eHST 6
Influence of coronal mass ejection on geomagnetic activity during 1988–1993
DOI: 10.1023/A:1021220005732 Bibcode: 2002EM&P...91....1S

Shrivastava, Pankaj Kumar; Singh, G. N.

The most rapid and dramatic evolution in the solar corona occurs in events now known as Coronal Mass Ejections (CMEs). There have considerable importance for our understanding of the evolution of the mass and energy injected into the interplanetary medium. In this work, we have studied the relation of CMEs with geomagnetic activity for the period …

2002 Earth Moon and Planets
SOHO 6
Contribution to the search for binaries among Am stars - III. HD 7119: a double-lined spectroscopic binary and a triple system
DOI: 10.1046/j.1365-8711.2002.05842.x Bibcode: 2002MNRAS.336.1043C

Udry, S.; Ginestet, N.; Prieur, J. -L. +1 more

Radial velocity observations of HD 7119 with the CORAVEL instrument at Observatoire de Haute-Provence are reported. Known as an Amδδ Del metallic-line star, HD 7119 was included in our spectroscopic survey of Am-type stars, the purpose of which was to determine the frequency of binaries in this stellar family. This object is found to be a double-l…

2002 Monthly Notices of the Royal Astronomical Society
Hipparcos 6
Detecting low amplitude periodicities with HIPPARCOS
DOI: 10.1051/0004-6361:20020146 Bibcode: 2002A&A...385..533K

Kallinger, T.; Weiss, W. W.

The HIPPARCOS and TYCHO catalogues have proven to be a very powerful source for detection of variability in stars. The photometric errors for individual measurements are typically of the order of a few millimagnitudes. Amplitudes for periodic variability of stars and based on HIPPARCOS data are published which are of the same order. An example cou…

2002 Astronomy and Astrophysics
Hipparcos 6
A Polarimetric Survey for Dust in 47 Tucanae
DOI: 10.1086/340471 Bibcode: 2002AJ....123.3263F

Forte, Juan C.; Vega, E. Irene; Cellone, Sergio A. +3 more

We present linear polarization measurements in the V band for 77 stars in the field of the globular cluster 47 Tucanae (NGC 104) and for 14 regions free of bright stars, located along an elliptical isophotal contour of the cluster, as well as UBVRI measurements for the cluster nucleus. The observations show variable foreground polarization that, o…

2002 The Astronomical Journal
eHST 6
The multimode pulsation of the delta Scuti star V784 Cassiopeae
DOI: 10.1051/0004-6361:20021058 Bibcode: 2002A&A...394...97K

Thomson, J. R.; Derekas, A.; Garrido, R. +5 more

We present an analysis of new Johnson and Strömgren photometric and medium-resolution spectroscopic observations of the delta Scuti type variable star V784 Cassiopeae. The data were obtained in three consecutive years between 1999 and 2001. The period analysis of the light curve resulted in the detection of four frequencies ranging from 9.15 d

2002 Astronomy and Astrophysics
Hipparcos 6
Observations of shock acceleration signatures by Ulysses: the 04:08:16, day147, 1991 UT shock
DOI: 10.1016/S1364-6826(02)00009-3 Bibcode: 2002JASTP..64..527M

Sarris, E. T.; Anagnostopoulos, G. C.; Marhavilas, P. K.

We analyze the acceleration signatures of energetic ions (E>50keV) and electrons (E>30keV) observed on day 147, 1991 UT in the vicinity of the surface of a fast-mode hydromagnetic shock, using fine time resolution measurements by the HI-SCALE instrument onboard the Ulysses spacecraft. The observations present strong evidence for the accelera…

2002 Journal of Atmospheric and Solar-Terrestrial Physics
Ulysses 6
Timing analysis of the core of the Crab-like SNR G21.5-0.9
DOI: 10.1051/0004-6361:20011839 Bibcode: 2002A&A...383..916L

Mereghetti, S.; La Palombara, N.

The Crab-like SNR G21.5-0.9 was observed in the X-ray band (0.5-10 keV) by the XMM-Newton satellite for over 100 ks. The large effective area of the EPIC instrument has allowed us to perform a deep search for pulsations from the central core of . No pulsations were found with upper limits on the pulsed fraction between 7.5% and 40% (depending on f…

2002 Astronomy and Astrophysics
XMM-Newton 6
Quasi-molecular lines in Lyman wings of cool DA white dwarfs. Application to FUSE observations of G 231-40
DOI: 10.1051/0004-6361:20021141 Bibcode: 2002A&A...394..647H

Ferlet, R.; Lacour, S.; Vidal-Madjar, A. +3 more

We present new theoretical calculations of the total line profiles of Lyman alpha and Lyman beta which include perturbations by both neutral hydrogen and protons and all possible quasi-molecular states of H2 and H2+. They are used to improve theoretical modeling of synthetic spectra for cool DA white dwarfs. We com…

2002 Astronomy and Astrophysics
IUE 6
The spectroscopic binaries 21 Her and gamma Gem
DOI: 10.1051/0004-6361:20011746 Bibcode: 2002A&A...383..558L

Korotin, S. A.; Andrievsky, S. M.; Lehmann, H. +5 more

In the framework of a search campaign for short-term oscillations of early-type stars we analysed recently obtained spectroscopic and photometric observations of the early A-type spectroscopic binaries 21 Her and gamma Gem. From the radial velocities of 21 Her we derived an improved orbital period and a distinctly smaller eccentricity in compariso…

2002 Astronomy and Astrophysics
Hipparcos 6