Search Publications

Constraining the population of cosmic ray protons in cooling flow clusters with γ-ray and radio observations: Are radio mini-halos of hadronic origin?
DOI: 10.1051/0004-6361:20031464 Bibcode: 2004A&A...413...17P

Enßlin, T. A.; Pfrommer, C.

We wish to constrain the cosmic-ray proton (CRp) population in galaxy clusters. By hadronic interactions with the thermal gas of the intra-cluster medium (ICM), the CRp produce γ-rays for which we develop an analytic formalism to deduce their spectral distribution. Assuming the CRp-to-thermal energy density ratio XCRp and the CRp spectr…

2004 Astronomy and Astrophysics
INTEGRAL 249
Emergence of magnetic flux from the convection zone into the corona
DOI: 10.1051/0004-6361:20035934 Bibcode: 2004A&A...426.1047A

O'Shea, E.; Galsgaard, K.; Moreno-Insertis, F. +2 more

Numerical experiments of the emergence of magnetic flux from the uppermost layers of the solar interior to the photosphere and its further eruption into the low atmosphere and corona are carried out. We use idealized models for the initial stratification and magnetic field distribution below the photosphere similar to those used for multidimension…

2004 Astronomy and Astrophysics
SOHO 233
XMM-Newton EPIC observations of 21 low-redshift PG quasars
DOI: 10.1051/0004-6361:20047108 Bibcode: 2004A&A...422...85P

Porquet, D.; Reeves, J. N.; Brinkmann, W. +1 more

We present an X-ray spectral analysis of 21 low redshift quasars observed with XMM-Newton EPIC. All the sources are Palomar Green quasars with redshifts between 0.05 and 0.4 and have low Galactic absorption along the line-of-sight. A large majority of quasars in the sample (19/21) exhibit a significant soft excess below ∼1-1.5 keV, whilst two obje…

2004 Astronomy and Astrophysics
XMM-Newton 233
2MASS NIR photometry for 693 candidate globular clusters in M 31 and the Revised Bologna Catalogue
DOI: 10.1051/0004-6361:20035632 Bibcode: 2004A&A...416..917G

Bellazzini, M.; Galleti, S.; Federici, L. +2 more

We have identified in the 2MASS database 693 known and candidate globular clusters in M 31. The 2MASS J, H, K magnitudes of these objects have been transformed to the same homogeneous photometric system of existing near infrared photometry of M 31 globulars, finally yielding J, H, K integrated photometry for 279 confirmed M 31 clusters, 406 unconf…

2004 Astronomy and Astrophysics
eHST 223
Automated recognition of coronal mass ejections (CMEs) in near-real-time data
DOI: 10.1051/0004-6361:20041302 Bibcode: 2004A&A...425.1097R

Berghmans, D.; Robbrecht, E.

This paper presents a new method and first applications of software that we have developed to autonomously detect CMEs in image sequences from LASCO (Large Angle Spectrometric Coronagraph). The crux of the software is the detection of CMEs as bright ridges in (time, height) maps using the Hough transform. The next step employs clustering and morph…

2004 Astronomy and Astrophysics
SOHO 221
The host of GRB 030323 at z=3.372: A very high column density DLA system with a low metallicity
DOI: 10.1051/0004-6361:20040086 Bibcode: 2004A&A...419..927V

Pian, E.; Palazzi, E.; Kouveliotou, C. +29 more

We present photometry and spectroscopy of the afterglow of GRB 030323. VLT spectra of the afterglow show damped Lyα (DLA) absorption and low- and high-ionization lines at a redshift z=3.3718±0.0005. The inferred neutral hydrogen column density, log N(H I)=21.90±0.07, is larger than any (GRB- or QSO-) DLA H I column density inferred directly from L…

2004 Astronomy and Astrophysics
eHST 217
ISO spectroscopy of disks around Herbig Ae/Be stars
DOI: 10.1051/0004-6361:20040400 Bibcode: 2004A&A...426..151A

van den Ancker, M. E.; Acke, B.

We have investigated the infrared spectra of all 46 Herbig Ae/Be stars for which spectroscopic data are available in the ISO data archive. Our quantitative analysis of these spectra focuses on the emission bands at 3.3, 6.2, ``7.7'', 8.6 and 11.2 micron, linked to polycyclic aromatic hydrocarbons (PAHs), the nanodiamond-related features at 3.4 and…

2004 Astronomy and Astrophysics
ISO 212
On the nature of EIT waves, EUV dimmings and their link to CMEs
DOI: 10.1051/0004-6361:20040351 Bibcode: 2004A&A...427..705Z

Zhukov, A. N.; Auchère, F.

EIT waves and extreme-ultraviolet (EUV) dimmings attract particular attention as they frequently accompany Coronal Mass Ejections (CMEs). We present several examples of EIT waves and EUV dimmings with particular morphologies previously unreported in the literature. We report for the first time an EIT wave in the Fe XV (284 Å) bandpass of the SOHO/…

2004 Astronomy and Astrophysics
SOHO 202
Grids of model spectra for WN stars, ready for use
DOI: 10.1051/0004-6361:20040506 Bibcode: 2004A&A...427..697H

Hamann, W. -R.; Gräfener, G.

Grids of model atmospheres for Wolf-Rayet stars of the nitrogen sequence (WN subclass) are presented. The calculations account for the expansion of the atmosphere, non-LTE, clumping, and line blanketing from iron-group elements. Observed spectra of single Galactic WN stars can in general be reproduced consistently by this generation of models. The…

2004 Astronomy and Astrophysics
IUE 202
The structure and environment of young stellar clusters in spiral galaxies
DOI: 10.1051/0004-6361:20034533 Bibcode: 2004A&A...416..537L

Larsen, S. S.

A search for stellar clusters has been carried out in 18 nearby spiral galaxies, using archive images from the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. All of the galaxies have previously been imaged from the ground in UBVI. A catalogue of structural parameters, photometry and comments based on visual inspection of the cl…

2004 Astronomy and Astrophysics
eHST 194