Search Publications

Dense cores and star formation in the giant molecular cloud Vela C★★★
DOI: 10.1051/0004-6361/201935047 Bibcode: 2019A&A...628A.110M

Hill, T.; Weiss, A.; Csengeri, T. +12 more

Context. The Vela Molecular Ridge is one of the nearest (700 pc) giant molecular cloud (GMC) complexes hosting intermediate-mass (up to early B, late O stars) star formation, and is located in the outer Galaxy, inside the Galactic plane. Vela C is one of the GMCs making up the Vela Molecular Ridge, and exhibits both sub-regions of robust and sub-r…

2019 Astronomy and Astrophysics
Gaia Herschel 21
Thermal properties of slowly rotating asteroids: results from a targeted survey
DOI: 10.1051/0004-6361/201935129 Bibcode: 2019A&A...625A.139M

Geier, S.; Pál, A.; Thizy, O. +51 more

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the subsurface. However, thermal inertias have been determined mainly for fast rotators due to selection effects in the available photometry used to obtain shape models required for the…

2019 Astronomy and Astrophysics
AKARI 21
Homogeneity of 67P/Churyumov-Gerasimenko as seen by CONSERT: implication on composition and formation
DOI: 10.1051/0004-6361/201834865 Bibcode: 2019A&A...630A...6H

Blum, J.; Vincent, J. -B.; Kofman, W. +3 more

Context. After the landing of Philae, CONSERT probed the nucleus of 67P/Churyumov-Gerasimenko (67P) and observed no heterogeneities at metric scale within the probed part of the small lobe of 67P. Further studies have then quantified the observed homogeneity in terms of maximum permittivity contrast versus the typical size of heterogeneities.

2019 Astronomy and Astrophysics
Rosetta 21
The PLATO Solar-like Light-curve Simulator. A tool to generate realistic stellar light-curves with instrumental effects representative of the PLATO mission
DOI: 10.1051/0004-6361/201834822 Bibcode: 2019A&A...624A.117S

Smith, A. M. S.; Samadi, R.; Lebreton, Y. +10 more

Context. ESA's PLATO space mission, to be launched by the end of 2026, aims to detect and characterise Earth-like planets in their habitable zone using asteroseismology and the analysis of the transit events. The preparation of science objectives will require the implementation of hare-and-hound exercises relying on the massive generation of repre…

2019 Astronomy and Astrophysics
Gaia 21
The double blue-straggler sequence in NGC 2173: an artifact of field contamination
DOI: 10.1051/0004-6361/201834011 Bibcode: 2019A&A...621A..45D

Dalessandro, E.; Bastian, N.; Ferraro, F. R. +3 more

Here we discuss the case of the double blue straggler star (BSS) sequence recently detected in the young stellar cluster NGC 2173 in the Large Magellanic Cloud (LMC) by Li et al. (2018, ApJ, 856, 25). In order to investigate this feature we made use of two Hubble Space Telescope (HST) sets of observations, one (the same one used by Li et al.) prob…

2019 Astronomy and Astrophysics
eHST 20
High-precision analysis of binary stars with planets. I. Searching for condensation temperature trends in the HD 106515 system
DOI: 10.1051/0004-6361/201935352 Bibcode: 2019A&A...625A..39S

Jofré, E.; Jaque Arancibia, M.; Saffe, C. +4 more


Aims: We explore for the first time the probable chemical signature of planet formation in the remarkable binary system HD 106515. Star A hosts a massive long-period planet with 9 MJup detected by radial velocity, while there is no planet detected at the B star. We also refine stellar and planetary parameters by using non-solar-sca…

2019 Astronomy and Astrophysics
Gaia 20
Multi-season optical modulation phased with the orbit of the super-Earth 55 Cancri e
DOI: 10.1051/0004-6361/201936066 Bibcode: 2019A&A...631A.129S

Fossati, L.; Winn, J. N.; Lendl, M. +13 more

Context. 55 Cnc e is a transiting super-Earth orbiting a solar-like star with an orbital period of 17.7 h. In 2011, using the Microvariability and Oscillations in Stars (MOST) space telescope, a quasi-sinusoidal modulation in flux was detected with the same period as the planetary orbit. The amplitude of this modulation was too large to be explain…

2019 Astronomy and Astrophysics
eHST 20
Probing Polaris' puzzling radial velocity signals. Pulsational (in-)stability, orbital motion, and bisector variations
DOI: 10.1051/0004-6361/201834703 Bibcode: 2019A&A...623A.146A

Anderson, R. I.

We investigate temporally changing variability amplitudes and the multi-periodicity of the type-I Cepheid Polaris using 161 high-precision radial velocity (RV) and bisector inverse span (BIS) measurements based on optical spectra recorded using Hermes at the 1.2 m Flemish Mercator telescope on La Palma, Canary Islands, Spain. Using an empirical te…

2019 Astronomy and Astrophysics
Gaia 20
Towards sub-kpc scale kinematics of molecular and ionized gas of star-forming galaxies at z ∼ 1
DOI: 10.1051/0004-6361/201935896 Bibcode: 2019A&A...631A..91G

Chisholm, J.; Schaerer, D.; Dessauges-Zavadsky, M. +4 more

We compare the molecular and ionized gas kinematics of two strongly lensed galaxies at z ∼ 1 that lie on the main sequence at this redshift. The observations were made with ALMA and MUSE, respectively. We derive the CO and [O II] rotation curves and dispersion profiles of these two galaxies. We find a difference between the observed molecular and …

2019 Astronomy and Astrophysics
eHST 20
Isochrone-cloud fitting of the extended main-sequence turn-off of young clusters
DOI: 10.1051/0004-6361/201936549 Bibcode: 2019A&A...632A..74J

Bastian, N.; Aerts, C.; Johnston, C. +1 more

Context. Extended main-sequence turn-offs (eMSTOs) are a commonly observed property of young clusters. A global theoretical interpretation for eMSTOs is still lacking, but stellar rotation is considered a necessary ingredient to explain eMSTOs.
Aims: We aim to assess the importance of core-boundary and envelope mixing in stellar interiors for…

2019 Astronomy and Astrophysics
eHST 20