Search Publications

From X-Ray Dips to Eclipse: Witnessing Disk Reformation in the Recurrent Nova U Sco
DOI: 10.1088/0004-637X/745/1/43 Bibcode: 2012ApJ...745...43N

Talavera, A.; Ness, J. -U.; Hernanz, M. +9 more

The tenth recorded outburst of the recurrent eclipsing nova U Sco was observed simultaneously in X-ray, UV, and optical by XMM-Newton on days 22.9 and 34.9 after the outburst. Two full passages of the companion in front of the nova ejecta were observed, as was the reformation of the accretion disk. On day 22.9, we observed smooth eclipses in UV an…

2012 The Astrophysical Journal
IUE XMM-Newton 45
Trajectories and Distribution of Interstellar Dust Grains in the Heliosphere
DOI: 10.1088/0004-637X/760/1/46 Bibcode: 2012ApJ...760...46S

Slavin, Jonathan D.; Reach, William T.; Müller, Hans-Reinhard +4 more

The solar wind carves a bubble in the surrounding interstellar medium (ISM) known as the heliosphere. Charged interstellar dust grains (ISDG) encountering the heliosphere may be diverted around the heliopause or penetrate it depending on their charge-to-mass ratio. We present new calculations of trajectories of ISDG in the heliosphere, and the dus…

2012 The Astrophysical Journal
Ulysses 45
Constraints on mantle plumes on Venus: Implications for volatile history
DOI: 10.1016/j.icarus.2011.09.011 Bibcode: 2012Icar..217..510S

Sotin, Christophe; Smrekar, Suzanne E.

The analysis of Venus' gravity field and topography suggests the presence of a small number of deep mantle plumes (∼9). This study predicts the number of plumes formed at the core-mantle boundary, their characteristics, and the production of partial melt from adiabatic decompression. Numerical simulations are performed using a 3D spherical code th…

2012 Icarus
VenusExpress 45
Determination of binary asteroid orbits with a genetic-based algorithm
DOI: 10.1051/0004-6361/201118408 Bibcode: 2012A&A...543A..68V

Berthier, J.; Marchis, F.; Vachier, F.


Aims: Over the past decade, discoveries of multiple and binary asteroid systems have played a significant role in our general understanding of small solar system bodies. Direct observations of satellites of asteroids are rare and difficult since they require the use of already over-subscribed facilities such as adaptive optics (AO) on large 8…

2012 Astronomy and Astrophysics
eHST 45
The dark GRB 080207 in an extremely red host and the implications for gamma-ray bursts in highly obscured environments
DOI: 10.1111/j.1365-2966.2011.19811.x Bibcode: 2012MNRAS.421...25S

Cenko, S. B.; Bloom, J. S.; Watson, D. +9 more

We present comprehensive X-ray, optical, near- and mid-infrared and submm observations of GRB 080207 and its host galaxy. The afterglow was undetected in the optical and near-infrared (nIR) implying an X-ray-to-optical spectral slope less than 0.3, identifying GRB 080207 as a dark burst. Swift X-ray observations show extreme absorption in the host…

2012 Monthly Notices of the Royal Astronomical Society
eHST 45
X-Ray and Optical Observations of A 0535+26
DOI: 10.1088/0004-637X/754/1/20 Bibcode: 2012ApJ...754...20C

Guiriec, S.; Coe, M. J.; McBride, V. A. +13 more

We present recent contemporaneous X-ray and optical observations of the Be/X-ray binary system A 0535+26 with the Fermi/Gamma-ray Burst Monitor (GBM) and several ground-based observatories. These new observations are put into the context of the rich historical data (since ~1978) and discussed in terms of the neutron-star-Be-disk interaction. The B…

2012 The Astrophysical Journal
INTEGRAL 45
Cool and warm dust emission from M 33 (HerM33es)
DOI: 10.1051/0004-6361/201219291 Bibcode: 2012A&A...543A..74X

Boquien, M.; Braine, J.; Beck, R. +24 more

In the framework of the open-time key program "Herschel M 33 extended survey (HerM33es)", we study the far-infrared emission from the nearby spiral galaxy M 33 in order to investigate the physical properties of the dust such as its temperature and luminosity density across the galaxy. Taking advantage of the unique wavelength coverage (100, 160, 2…

2012 Astronomy and Astrophysics
Herschel 44
VLT-SINFONI integral field spectroscopy of low-z luminous and ultraluminous infrared galaxies. I. Atlas of the 2D gas structure
DOI: 10.1051/0004-6361/201219372 Bibcode: 2012A&A...546A..64P

Colina, L.; Arribas, S.; Alonso-Herrero, A. +2 more

We present an atlas of a sample of local (z < 0.1) LIRGs (10) and ULIRGs (7) covering the luminosity range log(LIR/L) = 11.1-12.4. The atlas is based on near-infrared H (1.45-1.85 µm) and K-band (1.95-2.45 µm) VLT-SINFONI integral field spectroscopy (IFS). The atlas presents the ionised, partially ionised, and…

2012 Astronomy and Astrophysics
eHST 44
On the Link between Associated Mg II Absorbers and Star Formation in Quasar Hosts
DOI: 10.1088/0004-637X/748/2/131 Bibcode: 2012ApJ...748..131S

Shen, Yue; Ménard, Brice

A few percent of quasars show strong associated Mg II absorption, with velocities (v off) lying within a few thousand km s-1 from the quasar systemic redshift. These associated absorption line (AAL) systems are usually interpreted as absorbers that are either intrinsic to the quasar and its host, or arising from external gala…

2012 The Astrophysical Journal
eHST 44
The M 16 molecular complex under the influence of NGC 6611. Herschel's perspective of the heating effect on the Eagle Nebula
DOI: 10.1051/0004-6361/201219009 Bibcode: 2012A&A...542A.114H

Hill, T.; White, G. J.; Roussel, H. +25 more

We present Herschel images from the HOBYS key program of the Eagle Nebula (M 16) in the far-infrared and sub-millimetre, using the PACS and SPIRE cameras at 70 µm, 160 µm, 250 µm, 350 µm, 500 µm. M 16, home to the Pillars of Creation, is largely under the influence of the nearby NGC 6611 high-mass star cluster. The He…

2012 Astronomy and Astrophysics
Herschel 44