Search Publications

Metallicities in M dwarfs: Investigating different determination techniques
DOI: 10.1051/0004-6361/202141920 Bibcode: 2022A&A...658A.194P

Amado, P. J.; Caballero, J. A.; Reiners, A. +17 more

Deriving metallicities for solar-like stars follows well-established methods, but for cooler stars such as M dwarfs, the determination is much more complicated due to forests of molecular lines that are present. Several methods have been developed in recent years to determine accurate stellar parameters for these cool stars (Teff ≲ 4000…

2022 Astronomy and Astrophysics
Gaia 38
The iron and oxygen content of LMC Classical Cepheids and its implications for the extragalactic distance scale and Hubble constant. Equivalent width analysis with Kurucz stellar atmosphere models
DOI: 10.1051/0004-6361/202142441 Bibcode: 2022A&A...658A..29R

Mucciarelli, Alessio; Riess, Adam; Yuan, Wenlong +6 more

Context. Classical Cepheids are primary distance indicators and a crucial stepping stone in determining the present-day value of the Hubble constant H0 to the precision and accuracy required to constrain apparent deviations from the ΛCDM Concordance Cosmological Model.
Aims: We measured the iron and oxygen abundances of a statistic…

2022 Astronomy and Astrophysics
Gaia 38
Uncovering astrometric black hole binaries with massive main-sequence companions with Gaia
DOI: 10.1051/0004-6361/202141866 Bibcode: 2022A&A...658A.129J

Mazeh, T.; Faigler, S.; Shahaf, S. +6 more

Context. In the era of gravitational wave astrophysics and with the precise astrometry of billions of stellar sources, the hunt for compact objects is more alive than ever. Rarely seen massive binaries with a compact object are a crucial phase in the evolution towards compact object mergers. With the upcoming third Gaia data release (DR3), the fir…

2022 Astronomy and Astrophysics
Gaia 37
The GAPS Programme at TNG. XXXV. Fundamental properties of transiting exoplanet host stars
DOI: 10.1051/0004-6361/202243467 Bibcode: 2022A&A...664A.161B

Baratella, M.; Scandariato, G.; Pagano, I. +38 more

Context. Exoplanetary properties strongly depend on stellar properties: to know the planet with accuracy and precision it is necessary to know the star as accurately and precisely as possible.
Aims: Our immediate aim is to characterize in a homogeneous and accurate way a sample of 27 transiting planet-hosting stars observed within the Global …

2022 Astronomy and Astrophysics
Gaia 37
The GAPS Programme at TNG. XXXVIII. Five molecules in the atmosphere of the warm giant planet WASP-69b detected at high spectral resolution
DOI: 10.1051/0004-6361/202243854 Bibcode: 2022A&A...665A.104G

Pagano, I.; Fossati, L.; Poretti, E. +32 more

Context. The field of exo-atmospheric characterisation is progressing at an extraordinary pace. Atmospheric observations are now available for tens of exoplanets, mainly hot and warm inflated gas giants, and new molecular species continue to be detected, revealing a richer atmospheric composition than previously expected. Thanks to its warm equili…

2022 Astronomy and Astrophysics
Gaia 37
The Villafranca catalog of Galactic OB groups. II. From Gaia DR2 to EDR3 and ten new systems with O stars
DOI: 10.1051/0004-6361/202142364 Bibcode: 2022A&A...657A.131M

Maíz Apellániz, J.; Alfaro, E. J.; Barbá, R. H. +4 more

Context. This is the second paper of a series on Galactic OB groups that uses astrometric and photometric data from Gaia and spectral classifications from the Galactic O-Star Spectroscopic Survey (GOSSS) and the Library of Libraries of Massive-star high-Resolution spectra (LiLiMaRlin). The previous paper was based on the second Gaia data release (…

2022 Astronomy and Astrophysics
Gaia 37
Chemo-kinematics of the Milky Way spiral arms and bar resonances: Connection to ridges and moving groups in the solar vicinity
DOI: 10.1051/0004-6361/202141836 Bibcode: 2022A&A...663A..38K

Gerhard, Ortwin; Khoperskov, Sergey

Making use of a new high-resolution spiral galaxy simulation as well as Gaia DR2 and EDR3 data complemented by chemical abundances from the Galah DR3, APOGEE DR16, and LAMOST DR5 surveys, we explore the possible link between the Milky Way (MW) spiral arms, (R, vϕ) ridges, and moving groups in local vR-vϕ space. We …

2022 Astronomy and Astrophysics
Gaia 37
Radio footprints of a minor merger in the Shapley Supercluster: From supercluster down to galactic scales
DOI: 10.1051/0004-6361/202142048 Bibcode: 2022A&A...660A..81V

Di Gennaro, G.; Diego, J. M.; Rossetti, M. +29 more

Context. The Shapley Supercluster (⟨z⟩≈0.048) contains several tens of gravitationally bound clusters and groups, making it an ideal subject for radio studies of cluster mergers.
Aims: We used new high sensitivity radio observations to investigate the less energetic events of mass assembly in the Shapley Supercluster from supercluster down to…

2022 Astronomy and Astrophysics
XMM-Newton 37
Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
DOI: 10.1051/0004-6361/202243824 Bibcode: 2022A&A...665A..78S

Salvato, M.; Nandra, K.; Merloni, A. +15 more

Context. The extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) observatory is revolutionizing X-ray astronomy. The mission provides unprecedented samples of active galactic nuclei (AGN) and clusters of galaxies, with the potential of studying astrophysical properties of X-ray sources and …

2022 Astronomy and Astrophysics
Gaia 36
LIDA: The Leiden Ice Database for Astrochemistry
DOI: 10.1051/0004-6361/202244032 Bibcode: 2022A&A...668A..63R

van Dishoeck, E. F.; Rocha, W. R. M.; Rachid, M. G. +3 more

Context. High-quality vibrational spectra of solid-phase molecules in ice mixtures and for temperatures of astrophysical relevance are needed to interpret infrared observations toward protostars and background stars. Such data are collected worldwide by several laboratory groups in support of existing and upcoming astronomical observations. Over t…

2022 Astronomy and Astrophysics
ISO 36