Search Publications

Tentative detection of micron-sized forsterite grains in the proto-planetary disk surrounding HD 100453
DOI: 10.1051/0004-6361:20040420 Bibcode: 2004A&A...427..519V

Waters, L. B. F. M.; Dominik, C.; van Boekel, R. +4 more

We have re-analyzed the ISO-SWS spectrum of the intermediate mass pre-main-sequence star HD 100453. We confirm the weakness of the 10 µm amorphous silicate band. We have found strong indications of the presence of a crystalline silicate emission at 34 µm, which had escaped detection so far due to severe glitches in the data. The 23.5 a…

2004 Astronomy and Astrophysics
ISO 8
Meteoroid Streams Associated to Comets 9P/Tempel 1 and 67P/Churyumov-Gerasimenko
DOI: 10.1007/s11038-005-1640-0 Bibcode: 2004EM&P...95...75V

Jorda, L.; Lamy, P.; Vaubaillon, J.

The meteoroid streams associated to short-period comets 9P/Tempel 1 (the target of the Deep Impact mission). and 67P/Churyumov-Gerasimenko (the target of the Rosetta mission) are studied. Their structure is overwhelmingly under the control of Jupiter and repeated relatively close encounters cause a reversal of the direction of the spati…

2004 Earth Moon and Planets
Rosetta 8
The double radio source 3C 343.1: A galaxy-QSO pair with very different redshifts
DOI: 10.1051/0004-6361:20031745 Bibcode: 2004A&A...414L..37A

Burbidge, E. M.; Arp, H.; Burbidge, G.

The strong radio source 3C 343.1 consists of a galaxy and a QSO separated by no more than about 0.25''. The chance of this being an accidental superposition is conservatively ∼1×10-8. The z=0.344 galaxy is connected to the z=0.750 QSO by a radio bridge. The numerical relation between the two redshifts is that predicted from p…

2004 Astronomy and Astrophysics
eHST 8
Proper Motions of 59 766 Stars Absolutized Using Galaxies in 149 Sky Fields (PUL2)
DOI: 10.1134/1.1774399 Bibcode: 2004AstL...30..469B

Bobylev, V. V.; Shakht, N. A.; Bronnikova, N. M.

The PUL2 catalog has been photographically compiled in Pulkovo according to Deutch's plan. The catalog contains the mean coordinates of stars in the ICRS system at epoch J2000.0 and their original absolute proper motions. The photographic observations were performed with a normal astrograph. The first and second epochs of the photographic plates a…

2004 Astronomy Letters
Hipparcos 8
Dark baryons not in ancient halo white dwarfs
DOI: 10.1051/0004-6361:20040491 Bibcode: 2004A&A...426...65C

McCracken, H. J.; Reylé, C.; Robin, A. C. +5 more

Having ruled out the possibility that stellar objects are the main contributor of the dark matter embedding galaxies, microlensing experiments cannot exclude the hypothesis that a significant fraction of the Milky Way dark halo might be made of MACHOs with masses in the range 0.5-0.8 M. Ancient white dwarfs are generally considered the…

2004 Astronomy and Astrophysics
eHST 8
XMM-Newton Observation of the Narrow-Line QSO PHL 1092: Detection of a High and Variable Soft Component
DOI: 10.1086/423837 Bibcode: 2004ApJ...614..626D

Rao, A. R.; Dewangan, G. C.; Dasgupta, Surajit

We present results based on an XMM-Newton observation of the high-luminosity narrow-line QSO PHL 1092 performed in 2003 January. The 0.3-10 keV spectrum is well described by a model that includes a power law (Γ~2.1) and two blackbody components (kT~130 eV and kT~50 eV). The soft X-ray excess emission is featureless and contributes ~80% to the tota…

2004 The Astrophysical Journal
XMM-Newton 8
Two Active Nuclei in 3C 294
DOI: 10.1086/380096 Bibcode: 2004ApJ...600..626S

Stockton, Alan; Canalizo, Gabriela; Ridgway, Susan E. +1 more

The z=1.786 radio galaxy 3C 294 lies < 10" from a 12 mag star and has been the target of at least three previous investigations using adaptive optics (AO) imaging. A major problem in interpreting these results is the uncertainty in the precise alignment of the radio structure with the H- or K-band AO imaging. Here we report observations of the …

2004 The Astrophysical Journal
eHST 8
X-ray detections of two young bona-fide brown dwarfs
DOI: 10.1051/0004-6361:20040016 Bibcode: 2004A&A...424..619B

Bouy, H.

I report the detection of two bona-fide brown dwarfs by XMM-Newton: [GY92] 141 in the ρ-Ophiuchus star-forming region and DENIS J155601-233809 in the Upper Scorpius OB association. The two objects have been detected with luminosities of LX =8.35 ± 2.86 × 1028 erg s-1 and L

2004 Astronomy and Astrophysics
XMM-Newton 8
Magnetic signatures of Jupiter's bow shock during the Cassini flyby
DOI: 10.1029/2003JA010258 Bibcode: 2004JGRA..109.9S04A

Dougherty, Michele K.; Crary, F.; Young, D. T. +1 more

The bow shock crossings detected during the Cassini flyby of Jupiter occur at positions which imply that Jupiter's bow shock was relatively inflated during the early (before 2001, Day 3) and late (after 2001, Day 40) periods of the encounter. A variety of magnetic shock signatures are seen, corresponding to a wide range (15-75 degrees) in the angl…

2004 Journal of Geophysical Research (Space Physics)
Cassini 8
Cluster observations of a complex high-altitude cusp passage during highly variable IMF
DOI: 10.5194/angeo-22-3707-2004 Bibcode: 2004AnGeo..22.3707T

Balogh, A.; Lavraud, B.; Rème, H. +12 more

On 26 February 2001, the Cluster spacecraft were outbound over the Northern Hemisphere, at approximately 12:00 MLT, approaching the magnetosheath through the high-altitude (and exterior) cusp region. Due to macroscopic motions of the cusp, the spacecraft made multiple entries into the exterior cusp region before exiting into the magnetosheath, pre…

2004 Annales Geophysicae
Cluster 8