Search Publications

A compositional link between rocky exoplanets and their host stars
DOI: 10.1126/science.abg8794 Bibcode: 2021Sci...374..330A

Bitsch, Bertram; Sousa, Sérgio G.; Martioli, Eder +17 more

Stars and planets both form by accreting material from a surrounding disk. Because they grow from the same material, theory predicts that there should be a relationship between their compositions. In this study, we search for a compositional link between rocky exoplanets and their host stars. We estimate the iron-mass fraction of rocky exoplanets …

2021 Science
Gaia 131
A Large Fraction of Hydrogen-rich Supernova Progenitors Experience Elevated Mass Loss Shortly Prior to Explosion
DOI: 10.3847/1538-4357/abef05 Bibcode: 2021ApJ...912...46B

Cenko, S. Bradley; Duev, Dmitry A.; Riddle, Reed +45 more

Spectroscopic detection of narrow emission lines traces the presence of circumstellar mass distributions around massive stars exploding as core-collapse supernovae. Transient emission lines disappearing shortly after the supernova explosion suggest that the material spatial extent is compact and implies an increased mass loss shortly prior to expl…

2021 The Astrophysical Journal
Gaia 130
Internal mixing of rotating stars inferred from dipole gravity modes
DOI: 10.1038/s41550-021-01351-x Bibcode: 2021NatAs...5..715P

Bowman, Dominic M.; Aerts, Conny; Gebruers, Sarah +7 more

During most of their life, stars fuse hydrogen into helium in their cores. The mixing of chemical elements in the radiative envelope of stars with a convective core is able to replenish the core with extra fuel. If effective, such deep mixing allows stars to live longer and change their evolutionary path. Yet localized observations to constrain in…

2021 Nature Astronomy
Gaia 130
Lyman continuum leakage from low-mass galaxies with M < 108 M
DOI: 10.1093/mnras/stab612 Bibcode: 2021MNRAS.503.1734I

Chisholm, J.; Schaerer, D.; Thuan, T. X. +5 more

We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of nine low-mass star-forming galaxies at redshifts, z, in the range 0.3179-0.4524, with stellar masses $M_\star \, \lt $ 108 M and very high specific star-formation rates sSFR ~150-630 Gyr-1, aiming to study the depend…

2021 Monthly Notices of the Royal Astronomical Society
eHST 129
Dark matter local density determination: recent observations and future prospects
DOI: 10.1088/1361-6633/ac24e7 Bibcode: 2021RPPh...84j4901D

Widmark, A.; de Salas, Pablo F.

This report summarises progress made in estimating the local density of dark matter (ρDM,⊙), a quantity that is especially important for dark matter direct detection experiments. We outline and compare the most common methods to estimate ρDM,⊙ and the results from recent studies, including those that have benefited from the o…

2021 Reports on Progress in Physics
Gaia 128
Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy
DOI: 10.1051/0004-6361/202039084 Bibcode: 2021A&A...648A..24V

de Graauw, Th.; Liseau, R.; Braine, J. +50 more

Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it is difficult to observe from Earth. The Herschel Space Observatory provided unprecedented sensitivity as well as spatial and spectral resolution to study water. The Water In Star-forming regions with Herschel (WISH) key program was designed to observ…

2021 Astronomy and Astrophysics
Herschel 125
Atmospheric Rossiter-McLaughlin effect and transmission spectroscopy of WASP-121b with ESPRESSO
DOI: 10.1051/0004-6361/202039344 Bibcode: 2021A&A...645A..24B

Bouchy, F.; Rebolo, R.; Pallé, E. +41 more

Context. Ultra-hot Jupiters are excellent laboratories for the study of exoplanetary atmospheres. WASP-121b is one of the most studied; many recent analyses of its atmosphere report interesting features at different wavelength ranges.
Aims: In this paper we analyze one transit of WASP-121b acquired with the high-resolution spectrograph ESPRES…

2021 Astronomy and Astrophysics
Gaia 124
Extreme-UV quiet Sun brightenings observed by the Solar Orbiter/EUI
DOI: 10.1051/0004-6361/202140380 Bibcode: 2021A&A...656L...4B

Haberreiter, M.; Mierla, M.; Zhukov, A. N. +25 more

Context. The heating of the solar corona by small heating events requires an increasing number of such events at progressively smaller scales, with the bulk of the heating occurring at scales that are currently unresolved.
Aims: The goal of this work is to study the smallest brightening events observed in the extreme-UV quiet Sun.
Method…

2021 Astronomy and Astrophysics
SolarOrbiter 124
Gaia Early Data Release 3. Structure and properties of the Magellanic Clouds
DOI: 10.1051/0004-6361/202039588 Bibcode: 2021A&A...649A...7G

Prusti, T.; Mazeh, T.; Zucker, S. +417 more

Context. This work is part of the Gaia Data Processing and Analysis Consortium papers published with the Gaia Early Data Release 3 (EDR3). It is one of the demonstration papers aiming to highlight the improvements and quality of the newly published data by applying them to a scientific case.
Aims: We use the Gaia EDR3 data to study the struct…

2021 Astronomy and Astrophysics
Gaia eHST 122
Atacama Cosmology Telescope: Modeling the gas thermodynamics in BOSS CMASS galaxies from kinematic and thermal Sunyaev-Zel'dovich measurements
DOI: 10.1103/PhysRevD.103.063514 Bibcode: 2021PhRvD.103f3514A

Hilton, Matt; Sifón, Cristóbal; Battaglia, Nicholas +52 more

The thermal and kinematic Sunyaev-Zel'dovich effects (tSZ, kSZ) probe the thermodynamic properties of the circumgalactic and intracluster medium (CGM and ICM) of galaxies, groups, and clusters, since they are proportional, respectively, to the integrated electron pressure and momentum along the line of sight. We present constraints on the gas ther…

2021 Physical Review D
Herschel 122