Search Publications

Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation
DOI: 10.1051/0004-6361/202141546 Bibcode: 2022A&A...664A.130S

Ofek, E.; Marques Oliveira, J.; Sicardy, B. +85 more

Context. As part of our international program aimed at obtaining accurate physical properties of trans-Neptunian objects (TNOs), we predicted a stellar occultation by the TNO (38628) Huya of the star Gaia DR2 4352760586390566400 (mG = 11.5 mag) on March 18, 2019. After an extensive observational campaign geared at obtaining the astromet…

2022 Astronomy and Astrophysics
Gaia 12
CAPOS: The bulge Cluster APOgee Survey. III. Spectroscopic tomography of Tonantzintla 2
DOI: 10.1051/0004-6361/202141742 Bibcode: 2022A&A...658A.116F

Cohen, Roger E.; Beers, Timothy C.; Minniti, Dante +10 more

We performed the first detailed spectral analysis of red giant members of the relatively high-metallicity globular cluster (GC) Tononzintla 2 (Ton 2) using high-resolution near-infrared spectra collected with the Apache Point Observatory Galactic Evolution Experiment II survey (APOGEE-2), obtained as part of the bulge Cluster APOgee Survey. We inv…

2022 Astronomy and Astrophysics
Gaia 12
A multiwavelength study of the W33 Main ultracompact HII region
DOI: 10.1051/0004-6361/202140914 Bibcode: 2022A&A...664A.140K

Menten, K. M.; Khan, S.; Wyrowski, F. +7 more


Aims: The dynamics of ionized gas around the W33 Main ultracompact HII region is studied using observations of hydrogen radio recombination lines and a detailed multiwavelength characterization of the massive star-forming region W33 Main is performed.
Methods: We used the Giant Meterwave Radio Telescope (GMRT) to observe the H167α recomb…

2022 Astronomy and Astrophysics
Herschel 12
Tracking the 3D evolution of a halo coronal mass ejection using the revised cone model
DOI: 10.1051/0004-6361/202142942 Bibcode: 2022A&A...660A.144Z

Zhang, Q. M.


Aims: This paper aims to track the three-dimensional (3D) evolution of a full halo coronal mass ejection (CME) on 2011 June 21.
Methods: The CME results from a nonradial eruption of a filament-carrying flux rope in NOAA active region 11236. The eruption was observed in extreme-ultraviolet (EUV) wavelengths by the extreme-ultraviolet imag…

2022 Astronomy and Astrophysics
SOHO 12
Kepler-93: A testbed for detailed seismic modelling and orbital evolution of super-Earths around solar-like stars
DOI: 10.1051/0004-6361/202141083 Bibcode: 2022A&A...659A..56B

Bétrisey, J.; Buldgen, G.; Khan, S. +4 more

Context. The advent of space-based photometry missions such as CoRoT, Kepler and TESS has sparkled the rapid development of asteroseismology and its synergies with exoplanetology. In the near future, the advent of PLATO will further strengthen such multi-disciplinary studies. In that respect, testing asteroseismic modelling strategies and their im…

2022 Astronomy and Astrophysics
Gaia 12
The interstellar medium of high-redshift galaxies: Gathering clues from C III] and [C II] lines
DOI: 10.1051/0004-6361/202243336 Bibcode: 2022A&A...663A.172M

Maiolino, R.; Pentericci, L.; Ferrara, A. +5 more

Context. A tight relation between [C II] 158 µm line luminosity and the star formation rate (SFR) has been observed for local galaxies. At high redshift (z > 5), galaxies instead deviate downwards from the local Σ[C II] − ΣSFR relation. This deviation might be caused by different interstellar medium (ISM) properties …

2022 Astronomy and Astrophysics
eHST 12
Energetic proton back-precipitation onto the solar atmosphere in relation to long-duration gamma-ray flares
DOI: 10.1051/0004-6361/202142002 Bibcode: 2022A&A...658A..23H

Laitinen, T.; Dalla, S.; de Nolfo, G. A. +4 more

Context. Gamma-ray emission during long-duration gamma-ray flare (LDGRF) events is thought to be caused mainly by > 300 MeV protons interacting with the ambient plasma at or near the photosphere. Prolonged periods of the gamma-ray emission have prompted the suggestion that the source of the energetic protons is acceleration at a coronal mass ej…

2022 Astronomy and Astrophysics
SOHO 12
Probing Kepler's hottest small planets via homogeneous search and analysis of optical secondary eclipses and phase variations
DOI: 10.1051/0004-6361/202039037 Bibcode: 2022A&A...658A.132S

Scandariato, G.; Pagano, I.; Fossati, L. +5 more

Context. High-precision photometry can lead to the detection of secondary eclipses and phase variations of highly irradiated planets.
Aims: We performed a homogeneous search and analysis of optical occultations and phase variations of the most favorable ultra-short-period (USP) (P < 1 days) sub-Neptunes (Rp < 4 R)…

2022 Astronomy and Astrophysics
Gaia 12
Open clusters housing classical Cepheids in Gaia DR3
DOI: 10.1051/0004-6361/202244570 Bibcode: 2022A&A...668A..13H

Hao, C. J.; Xu, Y.; Lin, Z. H. +4 more

The latest Gaia Data Release 3 provides an opportunity to expand the census of Galactic open clusters harboring classical Cepheid variables, thereby bolstering the cosmic distance scale. A comprehensive analysis yielded a total of 50 classical Cepheids associated with 45 open clusters, of which 39 open cluster-classical Cepheid pairs are considere…

2022 Astronomy and Astrophysics
Gaia 12
Pulsating hydrogen-deficient white dwarfs and pre-white dwarfs observed with TESS. III. Asteroseismology of the DBV star GD 358
DOI: 10.1051/0004-6361/202142153 Bibcode: 2022A&A...659A..30C

Kepler, S. O.; Hermes, J. J.; Kawaler, S. D. +14 more

Context. The collection of high-quality photometric data by space telescopes, such as the completed Kepler mission and the ongoing TESS program, is revolutionizing the area of white-dwarf asteroseismology. Among the different kinds of pulsating white dwarfs, there are those that have He-rich atmospheres, and they are called DBVs or V777 Her variab…

2022 Astronomy and Astrophysics
Gaia 12