Search Publications

High-velocity extended molecular outflow in the star-formation dominated luminous infrared galaxy ESO 320-G030
DOI: 10.1051/0004-6361/201628875 Bibcode: 2016A&A...594A..81P

Colina, L.; Villar-Martín, M.; Planesas, P. +9 more

We analyze new high spatial resolution (~60 pc) ALMA CO(2-1) observations of the isolated luminous infrared galaxy ESO 320-G030 (d = 48 Mpc) in combination with ancillary Hubble Space Telescope optical and near infrared (IR) imaging, as well as VLT/SINFONI near-IR integral field spectroscopy. We detect a high-velocity (~450 km s-1) spat…

2016 Astronomy and Astrophysics
Herschel eHST 47
Sulphur molecules in the circumstellar envelopes of M-type AGB stars
DOI: 10.1051/0004-6361/201527943 Bibcode: 2016A&A...588A.119D

Olofsson, H.; Justtanont, K.; Black, J. H. +2 more


Aims: The sulphur compounds SO and SO2 have not been widely studied in the circumstellar envelopes of asymptotic giant branch (AGB) stars. By presenting and modelling a large number of SO and SO2 lines in the low mass-loss rate M-type AGB star R Dor, and modelling the available lines of those molecules in a further four …

2016 Astronomy and Astrophysics
Herschel 47
Close stellar conjunctions of α Centauri A and B until 2050 . An mK = 7.8 star may enter the Einstein ring of α Cen A in 2028
DOI: 10.1051/0004-6361/201629201 Bibcode: 2016A&A...594A.107K

Kervella, P.; Mignard, F.; Thévenin, F. +1 more

The rapid proper motion of the α Cen pair (≈3.7 arcsec yr-1) and its location close to the galactic plane on a rich stellar background combine constructively to make them excellent candidates for close stellar conjunctions with more distant stars. Adding new differential astrometry to archival data, we have refined the orbital parameter…

2016 Astronomy and Astrophysics
XMM-Newton 47
Gaia FGK benchmark stars: new candidates at low metallicities
DOI: 10.1051/0004-6361/201628268 Bibcode: 2016A&A...592A..70H

Gilmore, G.; Randich, S.; Soubiran, C. +10 more

Context. We have entered an era of large spectroscopic surveys in which we can measure, through automated pipelines, the atmospheric parameters and chemical abundances for large numbers of stars. Calibrating these survey pipelines using a set of "benchmark stars" in order to evaluate the accuracy and precision of the provided parameters and abunda…

2016 Astronomy and Astrophysics
Gaia 47
Search for associations containing young stars (SACY). VII. New stellar and substellar candidate members in the young associations
DOI: 10.1051/0004-6361/201628253 Bibcode: 2016A&A...590A..13E

Bayo, A.; Montes, D.; Sterzik, M. F. +5 more

Context. The young associations offer us one of the best opportunities to study the properties of young stellar and substellar objects and to directly image planets thanks to their proximity (<200 pc) and age (≈5-150 Myr). However, many previous works have been limited to identifying the brighter, more active members (≈1 M) owing to…

2016 Astronomy and Astrophysics
XMM-Newton 47
A HIFI view on circumstellar H2O in M-type AGB stars: radiative transfer, velocity profiles, and H2O line cooling
DOI: 10.1051/0004-6361/201628310 Bibcode: 2016A&A...591A..44M

Olofsson, H.; Justtanont, K.; De Beck, E. +4 more


Aims: We aim to constrain the temperature and velocity structures, and H2O abundances in the winds of a sample of M-type asymptotic giant branch (AGB) stars. We further aim to determine the effect of H2O line cooling on the energy balance in the inner circumstellar envelope.
Methods: We use two radiative-transfer co…

2016 Astronomy and Astrophysics
Herschel 47
Parallax and masses of α Centauri revisited
DOI: 10.1051/0004-6361/201527859 Bibcode: 2016A&A...586A..90P

Boffin, Henri M. J.; Pourbaix, Dimitri

Context. Despite the thorough work of van Leeuwen, the parallax of α Centauri is still far from being carved in stone. Any derivation of the individual masses is therefore uncertain, if not questionable. And yet, that does not prevent this system from being used for calibration purpose in several studies.
Aims: We aim for more accurate model-…

2016 Astronomy and Astrophysics
Hipparcos 46
The Lyman alpha reference sample. VII. Spatially resolved Hα kinematics
DOI: 10.1051/0004-6361/201527373 Bibcode: 2016A&A...587A..78H

Verhamme, Anne; Cannon, John M.; Hayes, Matthew +19 more

We present integral field spectroscopic observations with the Potsdam Multi-Aperture Spectrophotometer of all 14 galaxies in the z ~ 0.1 Lyman Alpha Reference Sample (LARS). We produce 2D line-of-sight velocity maps and velocity dispersion maps from the Balmer α (Hα) emission in our data cubes. These maps trace the spectral and spatial properties …

2016 Astronomy and Astrophysics
eHST 46
Detailed homogeneous abundance studies of 14 Galactic s-process enriched post-AGB stars: In search of lead (Pb)
DOI: 10.1051/0004-6361/201527430 Bibcode: 2016A&A...587A...6D

Van Winckel, H.; Kamath, D.; Karakas, A. I. +4 more

Context. This paper is part of a larger project in which we systematically study the chemical abundances of Galactic and extragalactic post-asymptotic giant branch (post-AGB) stars. The goal at large is to provide improved observational constraints to the models of the complex interplay between the AGB s-process nucleosynthesis and the associated …

2016 Astronomy and Astrophysics
AKARI 45
SPOTS: The Search for Planets Orbiting Two Stars. II. First constraints on the frequency of sub-stellar companions on wide circumbinary orbits
DOI: 10.1051/0004-6361/201628231 Bibcode: 2016A&A...593A..38B

Janson, M.; Desidera, S.; Bonavita, M. +4 more

A large number of direct imaging surveys for exoplanets have been performed in recent years, yielding the first directly imaged planets and providing constraints on the prevalence and distribution of wide planetary systems. However, like most of the radial velocity ones, these generally focus on single stars, hence binaries and higher-order multip…

2016 Astronomy and Astrophysics
eHST 45