Search Publications

Evidence for feedback and stellar-dynamically regulated bursty star cluster formation: the case of the Orion Nebula Cluster
DOI: 10.1051/0004-6361/201732151 Bibcode: 2018A&A...612A..74K

Kroupa, Pavel; Beccari, Giacomo; Jeřábková, Tereza +2 more

A scenario for the formation of multiple co-eval populations separated in age by about 1 Myr in very young clusters (VYCs, ages less than 10 Myr) and with masses in the range 600-20 000 M is outlined. It rests upon a converging inflow of molecular gas building up a first population of pre-main sequence stars. The associated just-formed…

2018 Astronomy and Astrophysics
Gaia 49
Molecular gas content in obscured AGN at z > 1
DOI: 10.1051/0004-6361/201833040 Bibcode: 2018A&A...619A..90P

Daddi, E.; Sargent, M. T.; Vignali, C. +11 more


Aims: The standard active galactic nuclei (AGN)-galaxy co-evolutionary scenario predicts a phase of deeply "buried" supermassive black hole growth coexisting with a starburst (SB) before feedback phenomena deplete the cold molecular gas reservoir of the galaxy and an optically luminous quasar (QSO) is revealed (called the SB-QSO evolutionary …

2018 Astronomy and Astrophysics
eHST 49
The chemistry of disks around T Tauri and Herbig Ae/Be stars
DOI: 10.1051/0004-6361/201732518 Bibcode: 2018A&A...616A..19A

Agúndez, Marcelino; Le Petit, Franck; Roueff, Evelyne +1 more

Context. Infrared and (sub-)millimeter observations of disks around T Tauri and Herbig Ae/Be stars point to a chemical differentiation, with a lower detection rate of molecules in disks around hotter stars.
Aims: We aim to investigate the underlying causes of the chemical differentiation indicated by observations and perform a comparative stu…

2018 Astronomy and Astrophysics
eHST 48
First detection of H2S in a protoplanetary disk. The dense GG Tauri A ring
DOI: 10.1051/0004-6361/201833766 Bibcode: 2018A&A...616L...5P

Beck, T.; Chapillon, E.; Wakelam, V. +8 more

Context. Studying molecular species in protoplanetary disks is very useful to characterize the properties of these objects, which are the site of planet formation.
Aims: We attempt to constrain the chemistry of S-bearing molecules in the cold parts of circumstellar disk of GG Tau A.
Methods: We searched for H2S, CS, SO, and SO…

2018 Astronomy and Astrophysics
Gaia 48
Combining low- to high-resolution transit spectroscopy of HD 189733b. Linking the troposphere and the thermosphere of a hot gas giant
DOI: 10.1051/0004-6361/201731244 Bibcode: 2018A&A...612A..53P

Piotto, Giampaolo; Pepe, Francesco; Heng, Kevin +8 more

Space-borne low- to medium-resolution (ℛ 102-103) and ground-based high-resolution spectrographs (ℛ 105) are commonly used to obtain optical and near infrared transmission spectra of exoplanetary atmospheres. In this wavelength range, space-borne observations detect the broadest spectral features (alkali doublets, …

2018 Astronomy and Astrophysics
eHST 48
The CARMENES search for exoplanets around M dwarfs. A Neptune-mass planet traversing the habitable zone around HD 180617
DOI: 10.1051/0004-6361/201833354 Bibcode: 2018A&A...618A.115K

Stahl, O.; Amado, P. J.; Bauer, F. F. +37 more

Despite their activity, low-mass stars are of particular importance for the search of exoplanets by the means of Doppler spectroscopy, as planets with lower masses become detectable. We report on the discovery of a planetary companion around HD 180617, a bright (J = 5.58 mag), low-mass (M = 0.45M) star of spectral type M2.5 V. The star…

2018 Astronomy and Astrophysics
Gaia 48
The Gaia-ESO Survey: properties of newly discovered Li-rich giants
DOI: 10.1051/0004-6361/201833027 Bibcode: 2018A&A...617A...4S

Gilmore, G.; Bayo, A.; Recio-Blanco, A. +41 more


Aims: We report 20 new lithium-rich giants discovered within the Gaia-ESO Survey, including the first Li-rich giant with an evolutionary stage confirmed by CoRoT (Convection, Rotation and planetary Transits) data. We present a detailed overview of the properties of these 20 stars.
Methods: Atmospheric parameters and abundances were deriv…

2018 Astronomy and Astrophysics
CoRoT Gaia 48
Possible 1 hour quasi-periodic oscillation in narrow-line Seyfert 1 galaxy MCG-06-30-15
DOI: 10.1051/0004-6361/201833629 Bibcode: 2018A&A...616L...6G

Ho, Luis C.; Gupta, Alok C.; Wiita, Paul J. +3 more

We found a possible 1 h quasi-periodic oscillation (QPO) in a 55 ks X-ray observation of the narrow-line Seyfert 1 galaxy MCG-06-30-15 made with the XMM-Newton EPIC/pn detector in the energy range 0.3-10 keV. We identify a total modulation of 16% in the light curve and find a ≃3670 s quasi-period using Lomb-Scargle periodogram (LSP) and weighted w…

2018 Astronomy and Astrophysics
XMM-Newton 48
Ubiquitous ram pressure stripping in the Coma cluster of galaxies
DOI: 10.1051/0004-6361/201833427 Bibcode: 2018A&A...618A.130G

Boselli, A.; Gavazzi, G.; Consolandi, G. +2 more

We report the detection of Hα trails behind three new intermediate-mass irregular galaxies in the NW outskirts of the nearby cluster of galaxies Abell 1656 (Coma). Hints that these galaxies possess an extended component were found in earlier, deeper Hα observations carried out with the Subaru telescope. However the lack of a simultaneous r-band ex…

2018 Astronomy and Astrophysics
XMM-Newton 48
Local growth of dust- and ice-mixed aggregates as cometary building blocks in the solar nebula
DOI: 10.1051/0004-6361/201630175 Bibcode: 2018A&A...611A..18L

Blum, J.; Lacerda, P.; Lorek, S.

Context. Comet formation by gravitational instability requires aggregates that trigger the streaming instability and cluster in pebble-clouds. These aggregates form as mixtures of dust and ice from (sub-)micrometre-sized dust and ice grains via coagulation in the solar nebula. Aim. We investigate the growth of aggregates from (sub-)micrometre-size…

2018 Astronomy and Astrophysics
Rosetta 48