Search Publications

Orbital Evidences for Dark-matter-free Milky Way Dwarf Spheroidal Galaxies
DOI: 10.3847/1538-4357/ab77be Bibcode: 2020ApJ...892....3H

Hammer, Francois; Babusiaux, Carine; Bonifacio, Piercarlo +4 more

The nature of Milky Way dwarf spheroidals (MW dSphs) has been questioned, in particular whether they are dominated by dark matter (DM). Here we investigate an alternative scenario, for which tidal shocks are exerted by the MW to DM-free dSphs after a first infall of their gas-rich progenitors, and for which theoretical calculations have been verif…

2020 The Astrophysical Journal
Gaia 31
New and improved rotational periods of magnetic CP stars from ASAS-3, KELT, and MASCARA data
DOI: 10.1093/mnras/staa462 Bibcode: 2020MNRAS.493.3293B

Paunzen, Ernst; Hümmerich, Stefan; Bernhard, Klaus

Magnetic chemically peculiar (mCP) stars allow the investigation of such diverse phenomena as atomic diffusion, magnetic fields, and stellar rotation. The aim of the present investigation is to enhance our knowledge of the rotational properties of mCP stars by increasing the sample of objects with accurately determined rotational periods. To this …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 31
Gravitational-wave Radiation of Double Degenerates with Extremely Low-mass White Dwarf Companions
DOI: 10.3847/1538-4357/ab7dc2 Bibcode: 2020ApJ...893....2L

Han, Zhanwen; Chen, Xuefei; Li, Zhenwei +3 more

Double degenerate (DD) systems are supposed to be significant gravitational-wave (GW) sources for future space-based GW detectors, e.g., the Laser Interferometer Space Antenna (LISA). Recently, one type of DD system with extremely low-mass WD (ELM WD; ≲ 0.30 M) companions was found in the ELM Survey. These companions have very short or…

2020 The Astrophysical Journal
Gaia 31
Evolution of the Alfvén Mach number associated with a coronal mass ejection shock
DOI: 10.1051/0004-6361/201936449 Bibcode: 2020A&A...633A..56M

Gallagher, Peter T.; Carley, Eoin P.; Maguire, Ciara A. +1 more

The Sun regularly produces large-scale eruptive events, such as coronal mass ejections (CMEs) that can drive shock waves through the solar corona. Such shocks can result in electron acceleration and subsequent radio emission in the form of a type II radio burst. However, the early-phase evolution of shock properties and its relationship to type II…

2020 Astronomy and Astrophysics
SOHO 31
Three short-period Jupiters from TESS. HIP 65Ab, TOI-157b, and TOI-169b
DOI: 10.1051/0004-6361/202037941 Bibcode: 2020A&A...639A..76N

Tamura, M.; Bouchy, F.; Henning, T. +74 more

We report the confirmation and mass determination of three hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HIP 65Ab (TOI-129, TIC-201248411) is an ultra-short-period Jupiter orbiting a bright (V = 11.1 mag) K4-dwarf every 0.98 days. It is a massive 3.213 ± 0.078 MJ planet in a grazing transit configu…

2020 Astronomy and Astrophysics
Gaia 30
The Lyman Alpha Reference Sample. X. Predicting Lyα Output from Star-forming Galaxies Using Multivariate Regression
DOI: 10.3847/1538-4357/ab7a91 Bibcode: 2020ApJ...892...48R

Hayes, Matthew; Östlin, Göran; Melinder, Jens +4 more

Understanding the production and escape of Lyα radiation from star-forming galaxies is a long-standing problem in astrophysics. The ability to predict the Lyα luminosity of galaxies would open up new ways of exploring the epoch of reionization (EOR) and estimating Lyα emission from galaxies in cosmological simulations where radiative transfer calc…

2020 The Astrophysical Journal
eHST 30
Transits of Known Planets Orbiting a Naked-eye Star
DOI: 10.3847/1538-3881/aba835 Bibcode: 2020AJ....160..129K

Butler, R. Paul; Kristiansen, Martti H.; Vanderburg, Andrew +45 more

Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well characterized and they preferentially orbit bright stars that are the targets of RV surveys. The Transiting Exoplanet Survey Satellite (TESS) provides an opportunity to sur…

2020 The Astronomical Journal
Gaia 30
Molecular complexity in pre-stellar cores: a 3 mm-band study of L183 and L1544
DOI: 10.1051/0004-6361/201936884 Bibcode: 2020A&A...633A.118L

Bizzocchi, Luca; Caselli, Paola; Vastel, Charlotte +4 more

Context. Pre-stellar cores (PSCs) are units of star formation. Besides representing early stages of the dynamical evolution leading to the formation of stars and planets, PSCs also provide a substrate for incipient chemical complexity in the interstellar space.
Aims: Our aim is to understand the influence of external conditions on the chemica…

2020 Astronomy and Astrophysics
Herschel 30
The BepiColombo Mercury Imaging X-Ray Spectrometer: Science Goals, Instrument Performance and Operations
DOI: 10.1007/s11214-020-00750-2 Bibcode: 2020SSRv..216..126B

Bunce, Emma J.; Muinonen, Karri; Kallio, Esa +68 more

The Mercury Imaging X-ray Spectrometer is a highly novel instrument that is designed to map Mercury's elemental composition from orbit at two angular resolutions. By observing the fluorescence X-rays generated when solar-coronal X-rays and charged particles interact with the surface regolith, MIXS will be able to measure the atomic composition of …

2020 Space Science Reviews
BepiColombo 30
Precise astrometry and diameters of asteroids from occultations - a data set of observations and their interpretation
DOI: 10.1093/mnras/staa3077 Bibcode: 2020MNRAS.499.4570H

Herald, David; Gault, David; Anderson, Robert +10 more

Occultations of stars by asteroids have been observed since 1961, increasing from a very small number to now over 500 annually. We have created and regularly maintain a growing data set of more than 5000 observed asteroidal occultations. The data set includes the raw observations, astrometry at the 1 mas level based on centre of mass or figure (no…

2020 Monthly Notices of the Royal Astronomical Society
AKARI 30