Search Publications

The dust environment of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361:20035806 Bibcode: 2004A&A...422..357F

Rauer, H.; Fulle, M.; Barbieri, C. +4 more

The new target of the ESA Rosetta Mission is comet 67P/Churyumov-Gerasimenko, which passed its last perihelion on 18 August 2002 and was well observed from fall 2002 to spring 2003. Its most prominent feature was a thin dust tail, which is best fitted by the Neck-Line model. Fits of the whole tail provide the dust environment of 67P during a year …

2004 Astronomy and Astrophysics
Rosetta 58
Chandra Observations of the Three Most Metal Deficient Blue Compact Dwarf Galaxies Known in the Local Universe, SBS 0335-052, SBS 0335-052W, and I Zw 18
DOI: 10.1086/382949 Bibcode: 2004ApJ...606..213T

Bauer, Franz E.; Thuan, Trinh X.; Izotov, Yuri I. +1 more

We present an X-ray study of the three most metal deficient blue compact dwarf (BCD) galaxies known in the local universe, based on deep Chandra observations of SBS 0335-052 (0.025 Zsolar), SBS 0335-052W (0.02 Zsolar), and I Zw 18 (0.02 Zsolar). All three are detected, with more than 90% of their X-ray emission ari…

2004 The Astrophysical Journal
eHST 58
On the light echo in V838 Mon
DOI: 10.1051/0004-6361:20034015 Bibcode: 2004A&A...414..223T

Tylenda, R.

We present a theoretical outline of the light echo phenomenon and results of simple numerical simulations and we study the available images of the light echo in V838 Mon obtained with HST. An investigation of the observed expansion of the light echo leads us to conclude that the distance to V838 Mon is ⪆5 kpc. From an analysis of the inner bright …

2004 Astronomy and Astrophysics
eHST 57
The Iron Unresolved Transition Array in Active Galactic Nuclei
DOI: 10.1086/382038 Bibcode: 2004ApJ...604..551N

Netzer, Hagai

The unresolved transition array (UTA) of iron M-shell ions is a prominent absorption feature in the X-ray spectrum of many active galactic nuclei (AGNs). Modeling photoionized plasmas in an attempt to match the observed silicon and oxygen lines fails to predict the level of ionization of iron as inferred by this feature. It is suggested that the d…

2004 The Astrophysical Journal
XMM-Newton 57
Jupiter's Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment
DOI: 10.1126/science.1100240 Bibcode: 2004Sci...305.1582K

Smith, M. D.; Strobel, D. F.; Lellouch, E. +39 more

The Composite Infrared Spectrometer observed Jupiter in the thermal infrared during the swing-by of the Cassini spacecraft. Results include the detection of two new stratospheric species, the methyl radical and diacetylene, gaseous species present in the north and south auroral infrared hot spots; determination of the variations with latitude of a…

2004 Science
Cassini 57
Hubble Space Telescope Observations of the Main Sequence of M4
DOI: 10.1086/383543 Bibcode: 2004AJ....127.2771R

Stetson, P. B.; Rich, R. M.; Shara, M. +8 more

We present new results from a photometric study of the main-sequence stars in M4 (NGC 6121=C1620-264), the closest globular cluster to the Sun. Multifield, multiepoch observations at approximately 1, 2, and 6 core radii were obtained with WFPC2 on the Hubble Space Telescope through either the F606W filter or the F555W (V) and F814W (I) filters. Th…

2004 The Astronomical Journal
eHST 57
XMM-Newton observations of the INTEGRAL X-ray transient IGR J17544-2619
DOI: 10.1051/0004-6361:20035940 Bibcode: 2004A&A...420..589G

Parmar, A. N.; Kuulkers, E.; González-Riestra, R. +2 more

On September 17, 2003 INTEGRAL discovered a bright transient source 3° from the Galactic Center, IGR J17544-2619. The field containing the transient was observed by XMM-Newton on March 17 and September 11 and 17, 2003. A bright source, at a position consistent with the INTEGRAL location, was detected by the European Photon Imagi…

2004 Astronomy and Astrophysics
INTEGRAL XMM-Newton 57
Asteroseismology of the β Cephei star ν Eridani - III. Extended frequency analysis and mode identification
DOI: 10.1111/j.1365-2966.2004.07791.x Bibcode: 2004MNRAS.351..324D

Handler, G.; De Ridder, J.; Heiter, U. +7 more

Using the large photometric and spectroscopic data sets of the ν Eridani multisite campaign given in our two recent papers (Aerts et al. and Handler et al.), we present an extended frequency analysis and a photometric mode identification. For the extended frequency analysis, we used an improved radial velocity time series, the second-moment time s…

2004 Monthly Notices of the Royal Astronomical Society
Hipparcos 57
UV-photoprocessing of interstellar ice analogs: Detection of hexamethylenetetramine-based species
DOI: 10.1051/0004-6361:20031447 Bibcode: 2004A&A...413..209M

Schutte, W. A.; Greenberg, J. M.; Muñoz Caro, G. M. +2 more

The physical conditions governing the dense cloud environment are reproduced in a high vacuum experimental setup at low temperature T ≈ 12 K. The accretion and photoprocessing of ices on grain surfaces is simulated by depositing an ice layer on a cold finger, while it is irradiated by ultraviolet (UV) photons. After irradiation the sample is slowl…

2004 Astronomy and Astrophysics
Rosetta 56
Revisiting the Origin of Impulsive Electron Events: Coronal Magnetic Restructuring
DOI: 10.1086/386319 Bibcode: 2004ApJ...609.1082M

Maia, Dalmiro Jorge Filipe; Pick, Monique

We revisit the impulsive beamlike particle events detected in situ from 1997 to 2000 by the Electron, Proton, and Alpha Monitor (EPAM) experiment on the Advanced Composition Explorer spacecraft. We study in detail a subset of events for which there are radio coronal observations from the Nançay Radioheliograph. EPAM measures electrons in the energ…

2004 The Astrophysical Journal
SOHO Ulysses 56