Search Publications

Internal motions in OB associations with Gaia DR2
DOI: 10.1093/mnras/staa454 Bibcode: 2020MNRAS.493.2339M

Melnik, A. M.; Dambis, A. K.

We study the motions inside 28 OB associations with the use of Gaia DR2 proper motions. The average velocity dispersion calculated for 28 OB associations including more than 20 stars with Gaia DR2 proper motion is σV = 4.5 km s-1. The median virial and stellar masses of OB associations are Mvir = 8.9 × 105

2020 Monthly Notices of the Royal Astronomical Society
Gaia 38
The CO-dark molecular gas mass in 30 Doradus
DOI: 10.1093/mnras/staa1106 Bibcode: 2020MNRAS.494.5279C

Lebouteiller, Vianney; Lee, Min-Young; Kruijssen, J. M. Diederik +16 more

Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular gas mass. However, despite being the most abundant molecule in the Universe, H2 is challenging to detect through direct observations and indirect methods have to be used to estimate the tot…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 38
Evidence for metallicity-dependent spin evolution in the Kepler field
DOI: 10.1093/mnras/staa3038 Bibcode: 2020MNRAS.499.3481A

Amard, Louis; Roquette, Julia; Matt, Sean P.

A curious rotation period distribution in the colour-magnitude-period diagram (CMPD) of the Kepler field was recently revealed, thanks to data from Gaia and Kepler spacecraft. It was found that redder and brighter stars are spinning slower than the rest of the main sequence. On the theoretical side, it was demonstrated that metallicity should affe…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 37
TESS observations of Be stars: a new interpretation
DOI: 10.1093/mnras/staa389 Bibcode: 2020MNRAS.493.2528B

Balona, L. A.; Ozuyar, D.

Light curves of 57 classical Be stars in TESS sectors 1-15 are examined. In most Be stars, the periodogram shows groups at a fundamental and one or more harmonics, which we attribute to rotation. In about 40 per cent of the stars, the group is just a single narrow or slightly broadened peak. In about 30 per cent, it consists of a multiple, closely…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 37
Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
DOI: 10.1093/mnras/staa3109 Bibcode: 2020MNRAS.499.4863P

Trujillo-Gomez, Sebastian; Crain, Robert A.; Kruijssen, J. M. D. +4 more

The ages and metallicities of globular clusters (GCs) are known to be powerful tracers of the properties of their progenitor galaxies, enabling their use in determining the merger histories of galaxies. However, while useful in separating GCs into individual accretion events, the orbits of GC groups themselves have received less attention as probe…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 37
Simultaneous TESS and NGTS transit observations of WASP-166 b
DOI: 10.1093/mnras/staa1075 Bibcode: 2020MNRAS.494.5872B

Wheatley, Peter J.; Bayliss, Daniel; Casewell, Sarah L. +21 more

We observed a transit of WASP-166 b using nine Next Generation Transit Survey (NGTS) telescopes simultaneously with the Transiting Exoplanet Survey Satellite (TESS) observations of the same transit. We achieved a photometric precision of 152 ppm per 30 min with the nine NGTS telescopes combined, matching the precision reached by TESS for the trans…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 37
Jet feedback and the photon underproduction crisis in SIMBA
DOI: 10.1093/mnras/staa3007 Bibcode: 2020MNRAS.499.2617C

Davé, Romeel; Christiansen, Jacob F.; Sorini, Daniele +1 more

We examine the impact of black hole jet feedback on the properties of the low-redshift intergalactic medium (IGM) in the SIMBA simulation, with a focus on the Lyα forest mean flux decrement DA. Without jet feedback, we confirm the photon underproduction crisis (PUC) in which ΓH I at $z$ = 0 must be increased by 6 times over t…

2020 Monthly Notices of the Royal Astronomical Society
eHST 37
Dynamical orbital classification of selected N-rich stars with Gaia Data Release 2 astrometry
DOI: 10.1093/mnras/staa1386 Bibcode: 2020MNRAS.495.4113F

Fernández-Trincado, José G.; Ortigoza-Urdaneta, Mario; Moreno, Edmundo +4 more

We have used the galaxy modelling algorithm GRAVPOT16, to explore the most probable orbital elements of a sample of 64 selected N-rich stars across the Milky Way. We use the newly measured proper motions from Gaia Data Release 2 with existing line-of-sight velocities from the second generation of the Apache Point Observatory Galactic Evolution Exp…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 37
TICs 167692429 and 220397947: the first compact hierarchical triple stars discovered with TESS
DOI: 10.1093/mnras/staa495 Bibcode: 2020MNRAS.493.5005B

Mitnyan, T.; Pál, A.; Klagyivik, P. +5 more

We report the discovery and complex analyses of the first two compact hierarchical triple star systems discovered with TESS in or near its southern continuous viewing zone during Year 1. Both TICs 167692429 and 220397947 were previously unknown eclipsing binaries, and the presence of a third companion star was inferred from eclipse timing variatio…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 37
WASP-52b. The effect of star-spot correction on atmospheric retrievals
DOI: 10.1093/mnras/stz3194 Bibcode: 2020MNRAS.491.5361B

Mikal-Evans, Thomas; Sing, David K.; López-Morales, Mercedes +13 more

We perform atmospheric retrievals on the full optical to infrared (0.3-5 µ m) transmission spectrum of the inflated hot Jupiter WASP-52b by combining HST/STIS, WFC3 IR, and Spitzer/IRAC observations. As WASP-52 is an active star that shows both out-of-transit photometric variability and star-spot crossings during transits, we account for the…

2020 Monthly Notices of the Royal Astronomical Society
eHST 36