Search Publications

Polarimetry of the Protoplanetary Nebula AFGL 2688
DOI: 10.1134/1.1704674 Bibcode: 2004ARep...48..288K

Miroshnichenko, A. S.; Klochkova, V. G.; Panchuk, V. E. +1 more

Our spectroscopic (with resolution R=75 000) and spectropolarimetric (R=15 000) observations with the 6-m telescope of the Special Astrophysical Observatory have enabled us to distinguish photospheric and circumstellar features in the optical spectrum of the bipolar protoplanetary nebula AFGL 2688 for the first time. The linear polarization of the…

2004 Astronomy Reports
eHST 14
Large-scale structure in the ELAIS S1 Survey
DOI: 10.1111/j.1365-2966.2004.07890.x Bibcode: 2004MNRAS.352...44G

Pozzi, F.; Vaccari, M.; Serjeant, S. +6 more

We present an analysis of the two-point angular correlation function of The European Large-Area Infrared Space Observatory (ELAIS) S1 survey. The survey covers 4 deg2 and contains 462 sources detected at 15 µm to a 5σ flux limit of 0.45 mJy. Using the 329 extragalactic sources not repeated in different observations, we detect a si…

2004 Monthly Notices of the Royal Astronomical Society
ISO 14
Meteorological predictions for the Beagle 2 mission to Mars
DOI: 10.1029/2003GL018966 Bibcode: 2004GeoRL..31.1703R

Michaels, Timothy I.; Haberle, Robert M.; Rafkin, Scot C. Randell

A general circulation and mesoscale model are used to predict the weather at the Beagle 2 landing site. The afternoon high temperature predicted by the general circulation model varies from 237 to 243 K over the duration of the primary mission. The overnight low temperature is 193 K +/- 2 K. Near surface wind speeds remain below 15 ms-1

2004 Geophysical Research Letters
MEx 14
Is the giant elliptical galaxy NGC 5018 a post-merger remnant?
DOI: 10.1051/0004-6361:20040282 Bibcode: 2004A&A...423..965B

Bressan, A.; Buson, L. M.; Burstein, D. +2 more

NGC 5018, one of the weakest UV emitters among giant ellipticals (gE) observed with IUE, appears to consist of an optical stellar population very similar to that of the compact, dwarf elliptical M 32, which is several magnitudes fainter in luminosity than NGC 5018 and whose stellar population is known to be ∼3 Gyr old. Here we show that the mid-UV…

2004 Astronomy and Astrophysics
IUE eHST 14
New observations from Cassini and Ulysses of Jovian VLF radio emissions
DOI: 10.1029/2003JA010233 Bibcode: 2004JGRA..109.9S08K

Gurnett, D. A.; Hospodarsky, G. B.; Kurth, W. S. +2 more

Simultaneous observations of Jupiter's so-called reradiated VLF radio emission by the Cassini and Ulysses spacecraft confirm that the emission is radiated into all directions in a pulse or strobe light-like fashion. These observations rule out a source that corotates with the planet. Observations of the same VLF emission component during the Cassi…

2004 Journal of Geophysical Research (Space Physics)
Cassini Ulysses 14
Astrometric monitoring of the binary brown dwarf DENIS-P J1228.2-1547
DOI: 10.1051/0004-6361:20041912 Bibcode: 2004A&A...428..205B

Martín, E. L.; Bouy, H.; Brandner, W. +4 more

We present astrometric monitoring data of the binary brown dwarf DENIS-P J1228.2-1547. The data have been obtained with the Hubble Space Telescope over a time span of 5.5 yr, and confirm that DENIS-P J1228.2-1547 is indeed a common proper motion, i.e., physical, binary. The data cover about 1/8th of the binary orbit, indicating an orbital period o…

2004 Astronomy and Astrophysics
eHST 14
A Detailed Study of Opacity in the Upper Atmosphere of Proxima Centauri
DOI: 10.1086/422803 Bibcode: 2004ApJ...612.1140C

Christian, D. J.; Mathioudakis, M.; Bloomfield, D. S. +2 more

We present far-UV and UV spectroscopic observations of Proxima Centauri obtained as part of our continued investigation into the optically thin approximation assumed for the transition regions of late-type stars. Significant opacity is found in the C III lines during both the quiescent and flaring states of Proxima Cen, with up to 70% of the expec…

2004 The Astrophysical Journal
eHST 14
Multiwavelength Properties of the X-Ray Sources in the Groth-Westphal Strip Field
DOI: 10.1086/420807 Bibcode: 2004AJ....127.3180M

Yamada, Toru; Griffiths, Richard E.; Sarajedini, Vicki +4 more

We summarize the multiwavelength properties of X-ray sources detected in the 80 ks XMM-Newton observation of the Groth-Westphal strip, a contiguous strip of 28 Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2) images. Among the ~150 X-ray sources detected in the XMM-Newton field of view, 23 are within the WFPC2 fields. Ten spectroscopic…

2004 The Astronomical Journal
XMM-Newton eHST 14
Acceleration of electrons by interacting CMEs
DOI: 10.1051/0004-6361:20031763 Bibcode: 2004A&A...415..755V

Odstrcil, D.; Vandas, M.

There is growing observational evidence that interaction of coronal mass ejections (CMEs) near the Sun is a common phenomenon, particularly during the solar cycle's maximum years. Recently, we performed 2.5-D MHD simulations of the interaction between two magnetic flux ropes. The aim was to provide some qualitative picture of the shock-cloud and c…

2004 Astronomy and Astrophysics
SOHO 14
Cluster observations of ELF/VLF signals generated by modulated heating of the lower ionosphere with the HAARP HF transmitter
DOI: 10.5194/angeo-22-2643-2004 Bibcode: 2004AnGeo..22.2643P

Platino, M.; Canu, P.; Bell, T. +5 more

Available from http://www.copernicus.org/site/EGU/annales/22/7/2643.htm?FrameEngine=false;

2004 Annales Geophysicae
Cluster 14