Search Publications

Gaia eclipsing binary and multiple systems. Supervised classification and self-organizing maps
DOI: 10.1051/0004-6361/201629710 Bibcode: 2017A&A...603A.117S

Rimoldini, L.; Holl, B.; Mowlavi, N. +6 more

Context. Large surveys producing tera- and petabyte-scale databases require machine-learning and knowledge discovery methods to deal with the overwhelming quantity of data and the difficulties of extracting concise, meaningful information with reliable assessment of its uncertainty. This study investigates the potential of a few machine-learning m…

2017 Astronomy and Astrophysics
Gaia Hipparcos 12
Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton
DOI: 10.1051/0004-6361/201629378 Bibcode: 2017A&A...597A..65M

Acero, Fabio; Maggi, Pierre


Aims: We present a study of the Galactic supernova remnant SNR G15.9+0.2 with archival XMM-Newton observations.
Methods: EPIC data are used to investigate the morphological and spectral properties of the remnant, searching in particular for supernova ejecta and Fe K line emission. By comparing the SNR's X-ray absorption column density wi…

2017 Astronomy and Astrophysics
XMM-Newton 12
Interstellar medium conditions in z 0.2 Lyman-break analogs
DOI: 10.1051/0004-6361/201730609 Bibcode: 2017A&A...606A..86C

Berta, S.; Magnelli, B.; Lutz, D. +16 more

We present an analysis of far-infrared (FIR) [CII] and [OI] fine structure line and continuum observations obtained with Herschel/PACS, and 12CO(1-0) observations obtained with the IRAM Plateau de Bure Interferometer, of Lyman-break analogs (LBAs) at z 0.2. The principal aim of this work is to determine the typical interstellar medium (…

2017 Astronomy and Astrophysics
Herschel ISO 12
The chemical structure of the Class 0 protostellar envelope NGC 1333 IRAS 4A
DOI: 10.1051/0004-6361/201630160 Bibcode: 2017A&A...603A..88K

Caux, E.; van der Tak, F. F. S.; Boogert, A. C. A. +2 more

Context. It is not well known what drives the chemistry of a protostellar envelope, in particular the role of the stellar mass and the protostellar outflows on the chemical enrichment of such environments.
Aims: We study the chemical structure of the Class 0 protostellar envelope NGC 1333 IRAS 4A in order to (I) investigate the influence of t…

2017 Astronomy and Astrophysics
Herschel 12
A search for pre- and proto-brown dwarfs in the dark cloud Barnard 30 with ALMA
DOI: 10.1051/0004-6361/201628510 Bibcode: 2017A&A...597A..17H

Ménard, F.; de Gregorio-Monsalvo, I.; Eiroa, C. +9 more

Context. The origin of brown dwarfs is still under debate. While some models predict a star-like formation scenario, others invoke a substellar mass embryo ejection, a stellar disk fragmentation, or the photo-evaporation of an external core due to the presence of massive stars.
Aims: The aim of our work is to characterize the youngest and low…

2017 Astronomy and Astrophysics
AKARI 12
XMM-Newton and INTEGRAL view of the hard state of EXO 1745-248 during its 2015 outburst
DOI: 10.1051/0004-6361/201629731 Bibcode: 2017A&A...603A..39M

Stella, L.; de Martino, D.; Rea, N. +10 more

Context. Transient low-mass X-ray binaries (LMXBs) often show outbursts that typically last a few weeks and are characterized by a high X-ray luminosity (Lx ≈ 1036-1038 erg s-1), while most of the time they are found in X-ray quiescence (LX ≈ 1031-1033 erg s-1)…

2017 Astronomy and Astrophysics
INTEGRAL XMM-Newton 12
CoRoT 223992193: Investigating the variability in a low-mass, pre-main sequence eclipsing binary with evidence of a circumbinary disk
DOI: 10.1051/0004-6361/201628483 Bibcode: 2017A&A...599A..27G

Aigrain, S.; Gandolfi, D.; Bouvier, J. +10 more

CoRoT 223992193 is the only known low-mass, pre-main sequence eclipsing binary that shows evidence of a circumbinary disk. The system displays complex photometric and spectroscopic variability over a range of timescales and wavelengths. Using two optical CoRoT runs from 2008 and 2011/2012 (spanning 23 and 39 days), along with infrared Spitzer 3.6 …

2017 Astronomy and Astrophysics
CoRoT 12
Suprathermal helium in corotating interaction regions: combined observations from SOHO/CELIAS/STOF and ACE/SWICS
DOI: 10.1051/0004-6361/201628641 Bibcode: 2017A&A...599A..13Y

Bochsler, P.; Klecker, B.; Berger, L. +4 more

Context. Energetic particle enhancements that are associated with corotating interaction regions (CIRs) are typically believed to arise from the sunward propagation of particles that are accelerated by CIR-driven shocks beyond 1 AU. It is expected that these sunward-travelling particles will lose energy and scatter, resulting in a turnover of the …

2017 Astronomy and Astrophysics
SOHO 12
Gaia eclipsing binary and multiple systems. A study of detectability and classification of eclipsing binaries with Gaia
DOI: 10.1051/0004-6361/201629957 Bibcode: 2017A&A...602A.110K

Rimoldini, L.; Holl, B.; Mowlavi, N. +5 more

Context. In the new era of large-scale astronomical surveys, automated methods of analysis and classification of bulk data are a fundamental tool for fast and efficient production of deliverables. This becomes ever more important as we enter the Gaia era.
Aims: We investigate the potential detectability of eclipsing binaries with Gaia using a…

2017 Astronomy and Astrophysics
Gaia 12
Simulated Galactic methanol maser distribution to constrain Milky Way parameters
DOI: 10.1051/0004-6361/201730681 Bibcode: 2017A&A...604A..72Q

Reid, M. J.; Quiroga-Nuñez, L. H.; van Langevelde, H. J. +1 more

Context. Using trigonometric parallaxes and proper motions of masers associated with massive young stars, the Bar and Spiral Structure Legacy (BeSSeL) survey has reported the most accurate values of the Galactic parameters so far. The determination of these parameters with high accuracy has a widespread impact on Galactic and extragalactic measure…

2017 Astronomy and Astrophysics
Gaia 12