Search Publications

Evolutionary signatures in complex ejecta and their driven shocks
DOI: 10.5194/angeo-22-3679-2004 Bibcode: 2004AnGeo..22.3679F

Farrugia, C.; Berdichevsky, D.

We examine interplanetary signatures of ejecta-ejecta interactions. To this end, two time intervals of inner-heliospheric (≤1AU) observations separated by 2 solar cycles are chosen where ejecta/magnetic clouds are in the process of interacting to form complex ejecta. At the Sun, both intervals are characterized by many coronal mass ejections (CMEs…

2004 Annales Geophysicae
SOHO 88
X-ray emission from the nuclei, lobes and hot-gas environments of two FR II radio galaxies
DOI: 10.1111/j.1365-2966.2004.08118.x Bibcode: 2004MNRAS.353..879C

Hardcastle, M. J.; Croston, J. H.; Birkinshaw, M. +1 more

We report on the detection of multiple components of X-ray emission from the two FR II radio galaxies, 3C 223 and 3C 284, based on new XMM-Newton observations. We attribute the detected X-ray emission from the lobes of both sources to inverse-Compton scattering of cosmic microwave background photons. With this model, we find that the magnetic fiel…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 88
The Globular Cluster Systems of Five Nearby Spiral Galaxies: New Insights from Hubble Space Telescope Imaging
DOI: 10.1086/421934 Bibcode: 2004ApJ...611..220C

Chandar, Rupali; Lee, Myung Gyoon; Whitmore, Bradley

We use available multifilter Hubble Space Telescope (HST) WFPC2 imaging of five (M81, M83, NGC 6946, M101, and M51, in order of distance) low-inclination, nearby spiral galaxies to study ancient star cluster populations. Combining rigorous selection criteria to reject contaminants (individual stars, background galaxies, and blends) with optical ph…

2004 The Astrophysical Journal
eHST 87
The diameter and evolutionary state of Procyon A. Multi-technique modeling using asteroseismic and interferometric constraints
DOI: 10.1051/0004-6361:20031527 Bibcode: 2004A&A...413..251K

Bordé, P.; Provost, J.; Berthomieu, G. +3 more

We report the angular diameter measurement obtained with the VINCI/VLTI instrument on the nearby star Procyon A (α CMi A, F5IV-V), at a relative precision of ± 0.9%. We obtain a uniform disk angular diameter in the K band of θUD = 5.376±0.047 mas and a limb darkened value of θLD = 5.448±0.053 mas. Together with the HIPPARCOS …

2004 Astronomy and Astrophysics
Hipparcos 87
The interstellar N2 abundance towards HD 124314 from far-ultraviolet observations
DOI: 10.1038/nature02614 Bibcode: 2004Natur.429..636K

Andersson, B. -G.; McCandliss, Stephan R.; Knauth, David C. +1 more

The abundance of interstellar molecular nitrogen (N2) is of considerable importance: models of steady-state gas-phase interstellar chemistry, together with millimetre-wavelength observations of interstellar N2H+ in dense molecular clouds predict that N2 should be the most abundant nitrogen-bearing molecu…

2004 Nature
eHST 87
Coronal plasma flows and magnetic fields in solar active regions. Combined observations from SOHO and NSO/Kitt Peak
DOI: 10.1051/0004-6361:20041060 Bibcode: 2004A&A...428..629M

Marsch, E.; Xia, L. D.; Wiegelmann, T.

During the early days of the SOHO mission, SUMER observed a few active regions (ARs) connected with sunspots on the Sun and took their images and spectra in various EUV emission lines. In addition to these spectroscopic data magnetograms of the photospheric footpoint regions of the AR loops were available from the MDI on SOHO and the National Sola…

2004 Astronomy and Astrophysics
SOHO 87
X-ray reprocessing in Seyfert galaxies: Simultaneous XMM-Newton/BeppoSAX observations
DOI: 10.1051/0004-6361:20047128 Bibcode: 2004A&A...422...65B

Perola, G. C.; Bianchi, S.; Guainazzi, M. +2 more

We selected a sample of eight bright unobscured (at least at the iron line energy) Seyfert galaxies observed simultaneously by XMM-Newton and BeppoSAX, taking advantage of the complementary characteristics of the two missions. The main results of our analysis can be summarized as follows: narrow neutral iron lines are confirmed to be an ubiquitous…

2004 Astronomy and Astrophysics
XMM-Newton 87
Dawn: A journey in space and time
DOI: 10.1016/j.pss.2003.06.013 Bibcode: 2004P&SS...52..465R

Russell, C. T.; Jaumann, R.; Keller, H. U. +18 more

By successively orbiting both 4 Vesta and 1 Ceres the Dawn mission directly addresses the long-standing goals of understanding the origin and evolution of the solar system. Ceres and Vesta are two complementary terrestrial protoplanets (one apparently ;wet; and the other ;dry;), whose accretion was probably terminated by the formation of Jupiter. …

2004 Planetary and Space Science
eHST 87
Going Slitless: Images of Forbidden-Line Emission Regions of Classical T Tauri Stars Observed with the Hubble Space Telescope
DOI: 10.1086/386317 Bibcode: 2004ApJ...609..261H

Edwards, Suzan; Hartigan, Patrick; Pierson, Rachel

We have observed five classical T Tauri stars known to have strong forbidden-line emission with STIS in slitless mode on the Hubble Space Telescope. This technique makes it possible to image jets within a few tens of AU of their exciting sources, a region of great interest for models of accretion disks and jets. Slitless images generate emission-l…

2004 The Astrophysical Journal
eHST 87
Imaging of the Supernova Remnant Cassiopeia A with the Multiband Imaging Photometer for Spitzer (MIPS)
DOI: 10.1086/422583 Bibcode: 2004ApJS..154..290H

Egami, E.; Gehrz, R. D.; Krause, O. +20 more

We present new images of the supernova remnant (SNR) Cas A observed in the 24 and 70 µm bands of the Spitzer Space Telescope (Spitzer). The IR emission correlates well with the Si X-ray and optical [S II] emission but poorly with either the synchrotron-dominated radio structure or the continuum X-ray emission. The IR is therefore dominated b…

2004 The Astrophysical Journal Supplement Series
ISO 87