Search Publications

The ACS survey of Galactic globular clusters. XII. Photometric binaries along the main sequence
DOI: 10.1051/0004-6361/201016384 Bibcode: 2012A&A...540A..16M

Moretti, A.; Anderson, J.; Milone, A. P. +15 more

Context. The fraction of binary stars is an important ingredient to interpret globular cluster dynamical evolution and their stellar population.
Aims: We investigate the properties of main-sequence binaries measured in a uniform photometric sample of 59 Galactic globular clusters that were observed by HST WFC/ACS as a part of the Globular Clu…

2012 Astronomy and Astrophysics
eHST 421
Cluster-formation in the Rosette molecular cloud at the junctions of filaments
DOI: 10.1051/0004-6361/201118566 Bibcode: 2012A&A...540L..11S

Hill, T.; André, Ph.; Arzoumanian, D. +31 more


Aims: For many years feedback processes generated by OB-stars in molecular clouds, including expanding ionization fronts, stellar winds, or UV-radiation, have been proposed to trigger subsequent star formation. However, hydrodynamic models including radiation and gravity show that UV-illumination has little or no impact on the global dynamica…

2012 Astronomy and Astrophysics
Herschel 306
Differential emission measures from the regularized inversion of Hinode and SDO data
DOI: 10.1051/0004-6361/201117576 Bibcode: 2012A&A...539A.146H

Hannah, I. G.; Kontar, E. P.


Aims: To demonstrate the capabilities of regularized inversion to recover differential emission measures (DEMs) from multi-wavelength observations provided by telescopes such as Hinode and SDO.
Methods: We develop and apply an enhanced regularization algorithm, used in RHESSI X-ray spectral analysis, to constrain the ill-posed inverse pr…

2012 Astronomy and Astrophysics
Hinode 296
The mean star formation rate of X-ray selected active galaxies and its evolution from z ~ 2.5: results from PEP-Herschel
DOI: 10.1051/0004-6361/201219258 Bibcode: 2012A&A...545A..45R

Berta, S.; Magnelli, B.; Nordon, R. +37 more

We study relationships between star-formation rate (SFR) and the accretion luminosity and nuclear obscuration of X-ray selected active galactic nuclei (AGNs) using a combination of deep far-infrared (FIR) and X-ray data in three key extragalactic survey fields (GOODS-South, GOODS-North and COSMOS), as part of the PACS Evolutionary Probe (PEP) prog…

2012 Astronomy and Astrophysics
Herschel 266
A Herschel view of the far-infrared properties of submillimetre galaxies
DOI: 10.1051/0004-6361/201118312 Bibcode: 2012A&A...539A.155M

Smail, I.; Berta, S.; Magnelli, B. +48 more

We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known spectroscopic redshifts and observed with the Herschel Space Observatory as part of the PACS Evolutionary Probe (PEP) and the Herschel Multi-tiered Extragalactic Survey (HerMES) guaranteed time key programmes. Our study makes use of the broad far-in…

2012 Astronomy and Astrophysics
Herschel 253
Rotational velocities of A-type stars. IV. Evolution of rotational velocities
DOI: 10.1051/0004-6361/201117691 Bibcode: 2012A&A...537A.120Z

Royer, F.; Zorec, J.

Context. In previous works of this series, we have shown that late B- and early A-type stars have genuine bimodal distributions of rotational velocities and that late A-type stars lack slow rotators. The distributions of the surface angular velocity ratio Ω/Ωcritcrit is the critical angular velocity) have peculiar shapes a…

2012 Astronomy and Astrophysics
Hipparcos 233
Water in star-forming regions with Herschel (WISH). II. Evolution of 557 GHz 110-101 emission in low-mass protostars
DOI: 10.1051/0004-6361/201118146 Bibcode: 2012A&A...542A...8K

Liseau, R.; van Dishoeck, E. F.; Bergin, E. A. +22 more

Context. Water is a key tracer of dynamics and chemistry in low-mass star-forming regions, but spectrally resolved observations have so far been limited in sensitivity and angular resolution, and only data from the brightest low-mass protostars have been published.
Aims: The first systematic survey of spectrally resolved water emission in 29 …

2012 Astronomy and Astrophysics
Herschel 232
The warm gas atmosphere of the HD 100546 disk seen by Herschel. Evidence of a gas-rich, carbon-poor atmosphere?
DOI: 10.1051/0004-6361/201118218 Bibcode: 2012A&A...541A..91B

van Dishoeck, E. F.; Bruderer, S.; Herczeg, G. J. +1 more

Context. With the Herschel Space Observatory, lines of simple molecules (C+, O, and high-J lines of CO, Jup ≳ 14) have been observed in the atmosphere of protoplanetary disks. When combined with ground-based data on [C i], all principle forms of carbon can be studied. These data allow us to test model predictions for the main…

2012 Astronomy and Astrophysics
Herschel IUE 229
Temporal variations in the evaporating atmosphere of the exoplanet HD 189733b
DOI: 10.1051/0004-6361/201219363 Bibcode: 2012A&A...543L...4L

Ehrenreich, D.; Lecavelier des Etangs, A.; Bourrier, V. +8 more

Atmospheric escape has been detected from the exoplanet HD 209458b through transit observations of the hydrogen Lyman-α line. Here we present spectrally resolved Lyman-α transit observations of the exoplanet HD 189733b at two different epochs. These HST/STIS observations show for the first time that there are …

2012 Astronomy and Astrophysics
eHST 229
CAIXA: a catalogue of AGN in the XMM-Newton archive. III. Excess variance analysis
DOI: 10.1051/0004-6361/201118326 Bibcode: 2012A&A...542A..83P

Bianchi, S.; Ponti, G.; Guainazzi, M. +4 more

Context. We report on the results of the first XMM-Newton systematic "excess variance" study of all the radio quiet, X-ray un-obscured AGN. The entire sample consist of 161 sources observed by XMM-Newton for more than 10 ks in pointed observations, which is the largest sample used so far to study AGN X-ray variability on time scales less than a da…

2012 Astronomy and Astrophysics
XMM-Newton 218