Search Publications

HIFI observations of water in the atmosphere of comet C/2008 Q3 (Garradd)
DOI: 10.1051/0004-6361/201014665 Bibcode: 2010A&A...518L.150H

Blommaert, J. A. D. L.; Küppers, M.; Thomas, N. +42 more

High-resolution far-infrared and sub-millimetre spectroscopy of water lines is an important tool to understand the physical and chemical properties of cometary atmospheres. We present observations of several rotational ortho- and para-water transitions in comet C/2008 Q3 (Garradd) performed with HIFI on Herschel. These observations have provided t…

2010 Astronomy and Astrophysics
Herschel 32
The youngest massive protostars in the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201014688 Bibcode: 2010A&A...518L..73S

van Loon, J. Th.; Okumura, K.; Hony, S. +19 more

We demonstrate the unique capabilities of Herschel to study very young luminous extragalactic young stellar objects (YSOs) by analyzing a central strip of the Large Magellanic Cloud obtained through the HERITAGE science demonstration program. We combine PACS 100 and 160, and SPIRE 250, 350, and 500 µm photometry with 2MASS (1.25-2.17 µ…

2010 Astronomy and Astrophysics
Herschel 32
γ Cassiopeiae: an X-ray Be star with personality
DOI: 10.1051/0004-6361/200811319 Bibcode: 2010A&A...512A..22L

Motch, C.; Smith, M. A.; Lopes de Oliveira, R.

An exciting unsolved problem in the study of high energy processes of early type stars concerns the physical mechanism for producing X-rays near the Be star γ Cassiopeiae. By now we know that this source and several “γ Cas analogs” exhibit an unusual hard thermal X-ray spectrum, compared both to normal massive stars and the non-…

2010 Astronomy and Astrophysics
XMM-Newton 32
A deep survey of the AKARI north ecliptic pole field . I. WSRT 20 cm radio survey description, observations and data reduction
DOI: 10.1051/0004-6361/200913366 Bibcode: 2010A&A...517A..54W

Im, M.; Lee, H. M.; White, G. J. +17 more


Aims: The Westerbork Radio Synthesis Telescope, WSRT, has been used to make a deep radio survey of an ~1.7 degree2 field coinciding with the AKARI north ecliptic pole deep field. The observations, data reduction and source count analysis are presented, along with a description of the overall scientific objectives.
Methods: The…

2010 Astronomy and Astrophysics
AKARI 32
The β Pictoris disk imaged by Herschel PACS and SPIRE
DOI: 10.1051/0004-6361/201014626 Bibcode: 2010A&A...518L.133V

Heras, A. M.; Walker, H. J.; Ivison, R. J. +40 more

We obtained Herschel PACS and SPIRE images of the thermal emission of the debris disk around the A5V star β Pic. The disk is well resolved in the PACS filters at 70, 100, and 160 µm. The surface brightness profiles between 70 and 160 µm show no significant asymmetries along the disk, and are compatible with 90% of the emission between …

2010 Astronomy and Astrophysics
Herschel 31
Testing adiabatic contraction of dark matter in fossil group candidates
DOI: 10.1051/0004-6361/201014328 Bibcode: 2010A&A...517A..52D

Arnaud, M.; Pratt, G. W.; Zibetti, S. +3 more

We present deep XMM-Newton observations and ESO WFI optical imaging of two X-ray-selected fossil group candidates, RXC J0216.7-4749 and RXC J2315.7-0222. Using the X-ray data, we derive total mass profiles under the hydrostatic equilibrium assumption. The central regions of RXC J0216.7-4749 are found to be dominated by an X-ray bright AGN, and alt…

2010 Astronomy and Astrophysics
XMM-Newton 31
A sample of [C II] clouds tracing dense clouds in weak FUV fields observed by Herschel
DOI: 10.1051/0004-6361/201015089 Bibcode: 2010A&A...521L..19P

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

The [C ii] fine-structure line at 158 µm is an excellent tracer of the warm diffuse gas in the ISM and the interfaces between molecular clouds and their surrounding atomic and ionized envelopes. Here we present the initial results from Galactic observations of terahertz C+ (GOT C+), a Herschel key project devoted to studying the […

2010 Astronomy and Astrophysics
Herschel 31
Spectro-photometric close pairs in GOODS-S: major and minor companions of intermediate-mass galaxies
DOI: 10.1051/0004-6361/201014236 Bibcode: 2010A&A...518A..20L

Pérez-González, P. G.; López-Sanjuan, C.; Gallego, J. +3 more


Aims: Recent work has shown that major mergers of disc galaxies can only account for 20% of the growth of the galaxy red sequence between z = 1 and z = 0. Our goal here is to provide merger frequencies that encompass both major and minor mergers, derived from close pair statistics. We aim to show that reliable close pair statistics can be der…

2010 Astronomy and Astrophysics
eHST 31
GAS in Protoplanetary Systems (GASPS). I. First results
DOI: 10.1051/0004-6361/201014595 Bibcode: 2010A&A...518L.127M

Pinte, C.; Ménard, F.; Duchêne, G. +49 more

Context. Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel Space Observatory allows for the study of the warm disc atmosphere, using far-infrared spectroscopy to measure gas content and excitation conditions, and far-IR photometry to constrain the dust distribut…

2010 Astronomy and Astrophysics
Herschel 31
Herschel-SPIRE observations of the disturbed galaxy NGC 4438
DOI: 10.1051/0004-6361/201014547 Bibcode: 2010A&A...518L..63C

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

We present Herschel-SPIRE observations of the perturbed galaxy NGC 4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped atomic and molecular hydrogen, supporting the idea that gas and dust are perturbed in a similar fas…

2010 Astronomy and Astrophysics
Herschel 31