Search Publications

Dwarf spheroidals in the M 81 group - Metallicity distribution functions and population gradients
DOI: 10.1051/0004-6361/200913364 Bibcode: 2010A&A...521A..43L

Grebel, E. K.; Koch, A.; Lianou, S.


Aims: We study the dwarf spheroidal galaxies in the nearby M 81 group in order to construct their photometric metallicity distributions and to investigate the potential presence of population gradients. We select all the dwarf spheroidals with available Hubble Space Telescope / Advanced Camera for Surveys archival observations, nine in total.…

2010 Astronomy and Astrophysics
eHST 40
First detection of ND in the solar-mass protostar IRAS16293-2422
DOI: 10.1051/0004-6361/201015102 Bibcode: 2010A&A...521L..42B

Falgarone, E.; Maret, S.; Henning, T. +64 more

Context. In the past decade, much progress has been made in characterising the processes leading to the enhanced deuterium fractionation observed in the ISM and in particular in the cold, dense parts of star forming regions such as protostellar envelopes. Very high molecular D/H ratios have been found for saturated molecules and ions. However, lit…

2010 Astronomy and Astrophysics
Herschel 40
[CII] observations of H2 molecular layers in transition clouds
DOI: 10.1051/0004-6361/201015091 Bibcode: 2010A&A...521L..18V

Li, D.; Goldsmith, P. F.; Langer, W. D. +3 more

We present the first results on the diffuse transition clouds observed in [CII] line emission at 158 µm (1.9 THz) towards Galactic longitudes near 340° (5 LOSs) & 20° (11 LOSs) as part of the HIFI tests and GOT C+ survey. Out of the total 146 [CII] velocity components detected by profile fitting we identify 53 as diffuse molecular clouds…

2010 Astronomy and Astrophysics
Herschel 40
On the influence of non-thermal pressure on the mass determination of galaxy clusters
DOI: 10.1051/0004-6361/200911855 Bibcode: 2010A&A...510A..76L

Laganá, T. F.; de Souza, R. S.; Keller, G. R.


Aims: Given that in most cases just thermal pressure is taken into account in the hydrostatic equilibrium equation to estimate galaxy cluster mass, the main purpose of this paper is to consider the contribution of all three non-thermal components to total mass measurements. The non-thermal pressure is composed by cosmic rays, turbulence and m…

2010 Astronomy and Astrophysics
XMM-Newton 40
Puzzling asteroid 21 Lutetia: our knowledge prior to the Rosetta fly-by
DOI: 10.1051/0004-6361/201013994 Bibcode: 2010A&A...515A..29B

Barucci, M. A.; Fornasier, S.; Fulchignoni, M. +5 more


Aims: A wide observational campaign was carried out in 2004-2009 that aimed to complete the ground-based investigation of Lutetia prior to the Rosetta fly-by in July 2010.
Methods: We obtained BVRI photometric and V-band polarimetric measurements over a wide range of phase angles, and visible and infrared spectra in the 0.4-2.4 µm …

2010 Astronomy and Astrophysics
Rosetta 40
Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705
DOI: 10.1051/0004-6361/201014580 Bibcode: 2010A&A...518L..58O

Elbaz, D.; Bock, J. J.; Clements, D. L. +56 more

We present Herschel SPIRE and PACS photometeric observations of the low metallicity (Z ~ 0.35 Z) nearby dwarf galaxy, NGC 1705, in six wavelength bands as part of the Dwarf Galaxy Survey guaranteed time Herschel key program. We confirm the presence of two dominant circumnuclear IR-bright regions surrounding the central super star clust…

2010 Astronomy and Astrophysics
Herschel 40
The energy spectrum of anomalous X-ray pulsars and soft gamma-ray repeaters
DOI: 10.1051/0004-6361/200911834 Bibcode: 2010A&A...518A..46T

Zezas, A.; Trümper, J. E.; Kylafis, N. D. +1 more

Context. Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) exhibit characteristic X-ray luminosities (both soft and hard) of around 1035 erg s-1 and characteristic power-law, hard X-ray spectra extending to about 200 keV. Two AXPs also exhibit pulsed radio emission.
Aims: Assuming that AXPs and SGRs accr…

2010 Astronomy and Astrophysics
INTEGRAL 40
GMRT observations of the Ophiuchus galaxy cluster
DOI: 10.1051/0004-6361/201014126 Bibcode: 2010A&A...514A..76M

Paltani, S.; Eckert, D.; Govoni, F. +4 more


Aims: Observations with the Very Large Array telescope at 1477 MHz revealed the presence of a radio mini-halo surrounding the faint central point-like radio source in the Ophiuchus cluster of galaxies. In this work we present a study of the radio emission from this cluster of galaxies at lower radio frequencies.
Methods: We observed the …

2010 Astronomy and Astrophysics
INTEGRAL 40
Herschel PACS and SPIRE imaging of CW Leonis
DOI: 10.1051/0004-6361/201014658 Bibcode: 2010A&A...518L.141L

Ivison, R. J.; Blommaert, J. A. D. L.; Olofsson, G. +25 more

Herschel PACS and SPIRE images have been obtained over a 30' × 30' area around the well-known carbon star CW Leo (IRC +10 216). An extended structure is found in an incomplete arc of 22' diameter, which is cospatial with the termination shock due to interaction with the interstellar medium (ISM) as defined by Sahai & Chronopoulos from ultravio…

2010 Astronomy and Astrophysics
Herschel 39
Polarimetric observations of comet 67P/Churyumov-Gerasimenko during its 2008-2009 apparition
DOI: 10.1051/0004-6361/201014167 Bibcode: 2010A&A...517A..86H

Lasue, J.; Sen, A. K.; Gupta, R. +2 more

Context. Remote observations of the light scattered by comet 67P/Churyumov-Gerasimenko dust coma are of major importance for determining the physical properties of the particles and prepare the rendezvous with the ESA/Rosetta spacecraft in 2014.
Aims: Light scattering and especially linear polarization observations allow comparison between di…

2010 Astronomy and Astrophysics
Rosetta 39