Search Publications

Five young δ Scuti stars in the Pleiades seen with Kepler/K2
DOI: 10.1093/mnras/stac240 Bibcode: 2022MNRAS.511.5718M

Li, Yaguang; Bedding, Timothy R.; White, Timothy R. +4 more

We perform mode identification for five δ Scuti stars in the Pleiades star cluster, using custom light curves from K2 photometry. By creating échelle diagrams, we identify radial and dipole mode ridges, comprising a total of 28 radial and 16 dipole modes across the five stars. We also suggest possible identities for those modes that lie offset fro…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Stellar and black hole assembly in z < 0.3 infrared-luminous mergers: intermittent starbursts versus super-Eddington accretion
DOI: 10.1093/mnras/stac980 Bibcode: 2022MNRAS.513.4770F

Lebouteiller, Vianney; Pearson, Chris; Clements, David L. +20 more

We study stellar and black hole mass assembly in a sample of 42 infrared-luminous galaxy mergers at z < 0.3 by combining results from radiative transfer modelling with archival measures of molecular gas and black hole mass. The ratios of stellar mass, molecular gas mass, and black hole mass to each other are consistent with those of massive gas…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 22
Improving blazar redshift constraints with the edge of the Ly α forest: 1ES 1553+113 and implications for observations of the WHIM
DOI: 10.1093/mnras/stab3331 Bibcode: 2022MNRAS.509.4330D

Narayanan, A.; Sameer; Charlton, J. +6 more

Blazars are some of the brightest ultraviolet (UV) and X-ray sources in the sky and are valuable probes of the elusive warm-hot intergalactic medium (WHIM; T ≃ 105-107 K). However, many of the brightest blazars - called BL Lac objects such as 1ES 1553+113 - have quasi-featureless spectra and poorly constrained redshifts. Here…

2022 Monthly Notices of the Royal Astronomical Society
eHST 22
The value-added catalogue of ASAS-SN eclipsing binaries: parameters of 30 000 detached systems
DOI: 10.1093/mnras/stac2520 Bibcode: 2022MNRAS.517.2190R

Kochanek, C. S.; Stanek, K. Z.; Thompson, Todd A. +6 more

Detached eclipsing binaries are a fundamental tool for measuring the physical parameters of stars that are effectively evolving in isolation. Starting from more than 40 000 eclipsing binary candidates identified by the All-Sky Automated Survey for Supernovae (ASAS-SN), we use PHOEBE to determine the sum of the fractional radii, the ratio of effect…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Chromosome maps of globular clusters from wide-field ground-based photometry
DOI: 10.1093/mnras/stac3086 Bibcode: 2022MNRAS.517.5687J

Milone, A. P.; Cordoni, G.; Marino, A. F. +10 more

Hubble Space Telescope (HST) photometry is providing an extensive analysis of globular clusters (GCs). In particular, the pseudo-two-colour diagram dubbed 'chromosome map (ChM)' allowed to detect and characterize their multiple populations with unprecedented detail. The main limitation of these studies is the small field of view of HST, which make…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
The white dwarf binary pathways survey - VIII. A post-common envelope binary with a massive white dwarf and an active G-type secondary star
DOI: 10.1093/mnras/stac2837 Bibcode: 2022MNRAS.517.2867H

Gänsicke, B. T.; Rebassa-Mansergas, A.; Raddi, R. +6 more

The white dwarf binary pathways survey is dedicated to studying the origin and evolution of binaries containing a white dwarf and an intermediate-mass secondary star of the spectral type A, F, G, or K (WD + AFGK). Here, we present CPD-65 264, a new post-common envelope binary with an orbital period of 1.37 d that contains a massive white dwarf ($0…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 22
Eclipsing white dwarf binaries in Gaia and the Zwicky Transient Facility
DOI: 10.1093/mnras/stab3293 Bibcode: 2022MNRAS.509.4171K

Belokurov, Vasily; Breedt, Elmé; Hodgkin, Simon +4 more

Gaia provided the largest ever catalogue of white dwarf stars. We use this catalogue, along with the third public data release of the Zwicky Transient Facility (ZTF), to identify new eclipsing white dwarf binaries. Our method exploits light-curve statistics and the box least-squares algorithm to detect periodic light-curve variability. The search …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Linking chromospheric activity and magnetic field properties for late-type dwarf stars
DOI: 10.1093/mnras/stac1291 Bibcode: 2022MNRAS.514.4300B

Petit, P.; Vidotto, A. A.; Jeffers, S. V. +9 more

Spectropolarimetric data allow for simultaneous monitoring of stellar chromospheric $\log {R^{\prime }_{\rm {HK}}}$ activity and the surface-averaged longitudinal magnetic field, Bl, giving the opportunity to probe the relationship between large-scale stellar magnetic fields and chromospheric manifestations of magnetism. We present $\lo…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22
Deriving ages and horizontal branch properties of integrated stellar populations
DOI: 10.1093/mnras/stac012 Bibcode: 2022MNRAS.511..341C

Conroy, Charlie; Cabrera-Ziri, Ivan

A major source of uncertainty in the age determination of old (~10 Gyr) integrated stellar populations is the presence of hot horizontal branch (HB) stars. Here, we describe a simple approach to tackle this problem, and show the performance of this technique that simultaneously models the age, abundances, and HB properties of integrated stellar po…

2022 Monthly Notices of the Royal Astronomical Society
eHST 22
Seismic modelling of a very young SPB star - KIC 8264293
DOI: 10.1093/mnras/stac168 Bibcode: 2022MNRAS.511.1529S

Walczak, Przemysław; Moździerski, Dawid; Daszyńska-Daszkiewicz, Jadwiga +1 more

KIC 8264293 is a fast-rotating B-type pulsator observed by Kepler satellite. Its photometric variability is mainly due to pulsations in high-order g modes. Besides, we detected a weak Hα emission. Thus, the second source of variability is the fluctuation in a disc around the star. The pulsational spectrum of KIC 8264293 reveals a frequency groupin…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 22