Search Publications

Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in the SMC galaxy
DOI: 10.1051/0004-6361/202243281 Bibcode: 2022A&A...666A.189R

Hamann, W. -R.; Gallagher, J. S.; Prinja, R. K. +9 more

Context. Massive stars are among the main cosmic engines driving the evolution of star-forming galaxies. Their powerful ionising radiation and stellar winds inject a large amount of energy in the interstellar medium. Furthermore, mass-loss (Ṁ) through radiatively driven winds plays a key role in the evolution of massive stars. Even so, the wind ma…

2022 Astronomy and Astrophysics
eHST 28
Observations of a Magellanic Corona
DOI: 10.1038/s41586-022-05090-5 Bibcode: 2022Natur.609..915K

Fox, Andrew J.; Wakker, Bart P.; Lehner, Nicolas +6 more

The Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC) are the closest massive satellite galaxies of the Milky Way. They are probably on their first passage on an infalling orbit towards our Galaxy1 and trace the continuing dynamics of the Local Group2. Recent measurements of a high mass for the LMC (Mhalo…

2022 Nature
eHST 28
Stellar Companions to TESS Objects of Interest: A Test of Planet-Companion Alignment
DOI: 10.3847/1538-3881/ac53a7 Bibcode: 2022AJ....163..160B

Howard, Andrew W.; Behmard, Aida; Dai, Fei

We present a catalog of stellar companions to host stars of Transiting Exoplanet Survey Satellite Objects of Interest (TOIs) identified from a marginalized likelihood ratio test that incorporates astrometric data from the Gaia Early Data Release 3 catalog (EDR3). The likelihood ratio is computed using a probabilistic model that incorporates parall…

2022 The Astronomical Journal
Gaia 28
Low-mass young stars in the Milky Way unveiled by DBSCAN and Gaia EDR3: Mapping the star forming regions within 1.5 kpc
DOI: 10.1051/0004-6361/202243580 Bibcode: 2022A&A...664A.175P

Alcalá, J. M.; Micela, G.; Jeffries, R. D. +6 more

Context. With an unprecedented astrometric and photometric data precision, Gaia EDR3 provides, for the first time, the opportunity to systematically detect and map, in the optical bands, the low-mass populations of the star forming regions (SFRs) in the Milky Way.
Aims: We aim to provide a catalogue of the Gαiα EDR3 data (photometry, proper m…

2022 Astronomy and Astrophysics
Gaia 28
Study of changes in the pulsation period of 148 Galactic Cepheid variables
DOI: 10.1093/mnras/stac115 Bibcode: 2022MNRAS.511.2125C

Szabados, L.; Cseh, B.; Molnár, L. +7 more

Investigating period changes of classical Cepheids through the framework of O - C diagrams provides a unique insight to the evolution and nature of these variable stars. In this work, the new or extended O - C diagrams for 148 Galactic classical Cepheids are presented. By correlating the calculated period change rates with the Gaia EDR3 colours, w…

2022 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL 28
TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS
DOI: 10.1051/0004-6361/202142540 Bibcode: 2022A&A...660A..86M

Moutou, C.; Carmona, A.; Donati, J. -F. +57 more

We report the detection and characterization of the transiting sub-Neptune TOI-1759 b, using photometric time series from the Transiting Exoplanet Survey Satellite (TESS) and near-infrared spectropolarimetric data from the Spectro-Polarimètre Infra Rouge (SPIRou) on the Canada-France-Hawaii Telescope. TOI-1759 b orbits a moderately active M0V star…

2022 Astronomy and Astrophysics
Gaia 28
The Local Group Mass in the Light of Gaia
DOI: 10.3847/2041-8213/ac5c42 Bibcode: 2022ApJ...928L...5B

Vasiliev, Eugene; Evans, N. Wyn; Strigari, Louis E. +3 more

High-accuracy proper motions (PMs) of M31 and other Local Group (LG) satellites have now been provided by the Gaia satellite. We revisit the timing argument to compute the total mass M of the LG from the orbit of the Milky Way and M31, allowing for the cosmological constant. We rectify a systematic effect caused by the presence of the Large Magell…

2022 The Astrophysical Journal
Gaia 28
Mapping the Complex Kinematic Substructure in the TW Hya Disk
DOI: 10.3847/1538-4357/ac88ca Bibcode: 2022ApJ...936..163T

Andrews, Sean M.; Bae, Jaehan; Bergin, Edwin A. +6 more

We present ALMA observations of CO J = 2 - 1 and CS J = 5 - 4 emission from the disk around TW Hydrae. Both molecules trace a predominantly Keplerian velocity structure, although a slowing of the rotation velocity is detected at the outer edge of the disk beyond ≈140 au in CO emission. This was attributed to the enhanced pressure support from the …

2022 The Astrophysical Journal
eHST 27
Measuring Elemental Abundances of JWST Target Stars for Exoplanet Characterization. I. FGK Stars
DOI: 10.3847/1538-3881/ac7de3 Bibcode: 2022AJ....164...87K

Wang, Ji; Kolecki, Jared R.

With the launch of the JWST, we will obtain more precise data for exoplanets than ever before. However, these data can only inform and revolutionize our understanding of exoplanets when placed in the larger context of planet-star formation. Therefore, gaining a deeper understanding of their host stars is equally important and synergistic with the …

2022 The Astronomical Journal
Gaia 27
Characterisation of Galactic carbon stars and related stars from Gaia EDR3
DOI: 10.1051/0004-6361/202243595 Bibcode: 2022A&A...664A..45A

de Laverny, P.; Figueras, F.; Romero-Gómez, M. +1 more

The third early Gaia data release (EDR3) has improved the accuracy of the astrometric parameters of numerous long-period variable (LPV) stars. Many of these stars are on the asymptotic giant branch (AGB), showing either a C-rich or O-rich envelope and are characterised by high luminosity, changing surface composition, and intense mass loss. This m…

2022 Astronomy and Astrophysics
Gaia 27