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A study of bright southern slowly pulsating B stars. II. The intrinsic frequencies
DOI: 10.1051/0004-6361:20021068 Bibcode: 2002A&A...393..965D

Aerts, C.; De Cat, P.

We present the results of detailed frequency analyses of a sample of thirteen confirmed slowly pulsating B stars. Our analysis is based on a combination of elaborate photometric and spectroscopic data-sets. The original sample consists of a mixture of five confirmed slowly pulsating B stars and twelve candidate slowly pulsating B stars discovered …

2002 Astronomy and Astrophysics
Hipparcos 109
A Second Planet Orbiting 47 Ursae Majoris
DOI: 10.1086/324336 Bibcode: 2002ApJ...564.1028F

Butler, R. Paul; Vogt, Steven S.; Fischer, Debra A. +2 more

Precise Doppler velocity measurements during 13 yr at Lick Observatory reveal the presence of two planets orbiting the star 47 UMa. The previously detected inner planet is confirmed by the newer velocities that yield a revised orbital period Pb=1089.0+/-2.9 days, Msini=2.54 MJ, and eccentricity eb=0.061+/-0.014. Th…

2002 The Astrophysical Journal
Hipparcos 109
Dissecting the Homunculus nebula around Eta Carinae with spatially resolved near-infrared spectroscopy
DOI: 10.1046/j.1365-8711.2002.05966.x Bibcode: 2002MNRAS.337.1252S

Smith, Nathan

Near-infrared emission lines are unique diagnostics of the geometry, structure, kinematics, and excitation of the circumstellar ejecta of η Carinae, and give clues to the nature of its wind. The infrared spectrum is a strong function of position in η Car's nebula, with a mix of intrinsic and reflected emission. Molecular hydrogen traces cool gas a…

2002 Monthly Notices of the Royal Astronomical Society
eHST 108
The Parallax and Proper Motion of RX J1856.5-3754 Revisited
DOI: 10.1086/339879 Bibcode: 2002ApJ...571..447K

van Kerkwijk, M. H.; Anderson, J.; Kaplan, D. L.

RX J1856.5-3754, a bright soft X-ray source believed to be the nearest thermally emitting neutron star, has commanded and continues to command intense interest from X-ray missions. One of the main goals is to determine the radius of this neutron star. An integral part of the determination is an accurate parallax. F. M. Walter analyzed Hubble Space…

2002 The Astrophysical Journal
eHST 108
The Cassini/Huygens Mission to the Saturnian System
DOI: 10.1023/A:1023609211620 Bibcode: 2002SSRv..104....1M

Lebreton, Jean-Pierre; Matson, Dennis L.; Spilker, Linda J.

The international Cassini/Huygens mission consists of the Cassini Saturn Orbiter spacecraft and the Huygens Titan Probe that is targeted for entry into the atmosphere of Saturn's largest moon, Titan. From launch on October 15, 1997 to arrival at Saturn in July 2004, Cassini/Huygens will travel over three billion kilometers. Once in orbit about Sat…

2002 Space Science Reviews
Cassini 107
Rotational velocities of A-type stars. I. Measurement of v sin i in the southern hemisphere
DOI: 10.1051/0004-6361:20011422 Bibcode: 2002A&A...381..105R

Royer, F.; Gerbaldi, M.; Faraggiana, R. +1 more

Within the scope of a Key Programme determining fundamental parameters of stars observed by HIPPARCOS, spectra of 525 B8 to F2-type stars brighter than V=8 have been collected at ESO. Fourier transforms of several line profiles in the range 4200-4500 Å are used to derive v sin i from the frequency of the first zero. Statistical analysis of the sam…

2002 Astronomy and Astrophysics
Hipparcos 107
On the association between type II radio bursts and CMEs
DOI: 10.1051/0004-6361:20020092 Bibcode: 2002A&A...384.1098C

Aurass, H.; Claßen, H. T.

Ground-based observations of metric (coronal) type II radio bursts are compared with observations of coronal mass ejections (CMEs) obtained by the LASCO coronagraph aboard SOHO and with decametric (interplanetary) type II bursts recorded by the WAVES instrument aboard Wind. The basic data sample comprises 63 metric type II radio bursts observed du…

2002 Astronomy and Astrophysics
SOHO 107
A multi-epoch spectrophotometric atlas of symbiotic stars
DOI: 10.1051/0004-6361:20011724 Bibcode: 2002A&A...383..188M

Munari, U.; Zwitter, T.

A multi-epoch, absolute-fluxed spectral atlas extending from about 3200 to 9000 Å is presented for 130 symbiotic stars, including members of the LMC, SMC and Draco dwarf galaxies. The fluxes are accurate to better than 5% as shown by comparison with Tycho and ground-based photometric data. The spectra of 40 reference objects (MKK cool giant standa…

2002 Astronomy and Astrophysics
Hipparcos 106
Multiplicity among chemically peculiar stars. II. Cool magnetic Ap stars
DOI: 10.1051/0004-6361:20021122 Bibcode: 2002A&A...394..151C

Babel, J.; Carrier, F.; Udry, S. +1 more

We present new orbits for sixteen Ap spectroscopic binaries, four of which might in fact be Am stars, and give their orbital elements. Four of them are SB2 systems: HD 5550, HD 22128, HD 56495 and HD 98088. The twelve other stars are: HD 9996, HD 12288, HD 40711, HD 54908, HD 65339, HD 73709, HD 105680, HD 138426, HD 184471, HD 188854, HD 200405 a…

2002 Astronomy and Astrophysics
Hipparcos 106
Deep Hubble Space Telescope WFPC2 Photometry of NGC 288. I. Binary Systems and Blue Stragglers
DOI: 10.1086/339222 Bibcode: 2002AJ....123.1509B

Fusi Pecci, Flavio; Rood, Robert T.; Messineo, Maria +2 more

We present the first results of a deep WFPC2 photometric survey of the loose galactic globular cluster NGC 288. The fraction of binary systems is estimated from the color distribution of objects near the main sequence (MS) with a method analogous to that introduced by Rubenstein & Bailyn. We have unequivocally detected a significant population…

2002 The Astronomical Journal
eHST 105