Search Publications

Submillimeter Emission from Type Ia Supernova Host Galaxies at z = 0.5
DOI: 10.1086/381487 Bibcode: 2004ApJ...603..489F

Farrah, D.; Fox, M.; Rowan-Robinson, M. +2 more

We present deep submillimeter observations of 17 galaxies at z=0.5 that are hosts of a Type Ia supernova. Two galaxies are detected directly, and the sample is detected statistically with a mean 850 µm flux of 1.01+/-0.33 mJy, which is 25%-135% higher than locally. We infer that the mean value of AV in normal galaxies at z=0.5 is …

2004 The Astrophysical Journal
eHST 13
A high-resolution study of the interstellar medium in the luminous IRAS galaxy Arp 193
DOI: 10.1111/j.1365-2966.2004.07647.x Bibcode: 2004MNRAS.350...66C

Clemens, M. S.; Alexander, P.

We present high-resolution multi-element radio-linked interferometer network (MERLIN) and Very Large Array (VLA) observations of the H I absorption towards the starburst nucleus of Arp 193 (IC 883, UGC 08387), a luminous IRAS merger. We compare the distribution of atomic gas with that of radio continuum emission, high-resolution CO data and near-i…

2004 Monthly Notices of the Royal Astronomical Society
eHST 13
The Solar and Interplanetary Causes of Space Storms in Solar Cycle 23
DOI: 10.1109/TPS.2004.830990 Bibcode: 2004ITPS...32.1411B

Bothmer, V.

2004 IEEE Transactions on Plasma Science
SOHO 13
SOHO CDS and SUMER observations of quiescent filaments and their interpretation
DOI: 10.1051/0004-6361:20034267 Bibcode: 2004A&A...420..307D

Parenti, S.; Del Zanna, G.; Chiuderi Drago, F.

Three quiescent filaments located at different positions on the solar disk were selected from the SOHO CDS data archive: one of them was also observed by SUMER in the raster mode. We investigate the filament-corona transition region (PCTR) emission, to determine whether it is indeed negligible, as found in one previously-analysed case. The observa…

2004 Astronomy and Astrophysics
SOHO 13
The Relationship of the Chromosphere to the Lower Solar Transition Region
DOI: 10.1086/421235 Bibcode: 2004ApJ...609.1153D

Doschek, G. A.; Mariska, J. T.; Akiyama, S.

We examine the intensity correlations among lower transition region emission lines of N III, N IV, N V, O II, O III, O IV, O V, S IV, and S V. We find strong intensity correlations, with 1 σ deviations in line intensity ratios less than about 35% on spatial scales of 1". For strong lines the percent deviations are significantly less than this. The…

2004 The Astrophysical Journal
SOHO 13
Chemical Composition of 15 Photometric Analogues of the Sun
DOI: 10.1134/1.1767216 Bibcode: 2004ARep...48..492G

Galazutdinov, G. A.; Bikmaev, I. F.; Galeev, A. I. +1 more

The results of a spectroscopic analysis of 15 stars that are photometric analogues of the Sun are reported. The effective temperatures and surface gravities in the stellar atmospheres are derived from published photometric indices and the HIPPARCOS parallaxes. The abundances of 33 elements ranging from lithium to europium are analyzed based on hig…

2004 Astronomy Reports
Hipparcos 13
Multipoint analysis of the spatio-temporal coherence of dayside O+ outflows with Cluster
DOI: 10.5194/angeo-22-2507-2004 Bibcode: 2004AnGeo..22.2507B

Klecker, B.; Rème, H.; Kistler, L. +5 more

Available from http://www.copernicus.org/site/EGU/annales/22/7/2507.htm?FrameEngine=false;

2004 Annales Geophysicae
Cluster 13
The analysis of Abell 1835 using a deprojection technique
DOI: 10.1051/0004-6361:20034006 Bibcode: 2004A&A...423...65J

Chen, Y.; Chen, L.; Lu, F. J. +2 more

We present the results from a detailed deprojection analysis of Abell 1835 as observed by XMM-Newton. If we fit the spectra with an isothermal plasma model, the deprojected temperature profile is flat in the outer region around 7.6 keV and decreases to ∼5.6 keV in the center, which may be connected with the gas cooling. In the central part, a two-…

2004 Astronomy and Astrophysics
XMM-Newton 13
Low-Ionization Emission-Line Regions around the Nucleus of the Seyfert Galaxy NGC 1068
DOI: 10.1093/pasj/56.5.723 Bibcode: 2004PASJ...56..723I

Hattori, Takashi; Ishigaki, Tsuyoshi; Sugai, Hajime +6 more

We present the results of tridimensional spectrophotometric observations of the central region of the Seyfert galaxy NGC 1068 obtained by using Kyoto tridimensional spectrograph I. A brief description of the instrument is presented. We have found the existence of low-ionized gas extending out of the ionization cone. It is characterized by higher (…

2004 Publications of the Astronomical Society of Japan
eHST 13
Identifying a black hole X-ray transient in M 31 with XMM-Newton and Chandra
DOI: 10.1051/0004-6361:20035661 Bibcode: 2004A&A...423..147B

Kolb, U.; Osborne, J. P.; Barnard, R.

Stochastic variability in two out of four XMM-Newton observations of XMMU J004303+4115 along with its power spectra and X-ray luminosities suggest a low-mass X-ray binary (LMXB) with a black hole primary. However, Chandra observations resolve the object into two point sources. We use data from 35 Chandra observations to analyse the contributions o…

2004 Astronomy and Astrophysics
XMM-Newton 13