Search Publications

The Photo-Astrometric vertical tracer density of the Milky Way - I. The method
DOI: 10.1093/mnras/stab3325 Bibcode: 2022MNRAS.511.2390E

Everall, Andrew; Boubert, Douglas; Grand, Robert J. J. +2 more

We introduce a method to infer the vertical distribution of stars in the Milky Way using a Poisson likelihood function, with a view to applying our method to the Gaia catalogue. We show how to account for the sample selection function and for parallax measurement uncertainties. Our method is validated against a simulated sample drawn from a model …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
Deep uGMRT observations of the ELAIS-North 1 field: statistical properties of radio-infrared relations up to z 2
DOI: 10.1093/mnras/stac1504 Bibcode: 2022MNRAS.514.4343S

Datta, Abhirup; Basu, Aritra; Sinha, Akriti +1 more

Comprehending the radio-infrared (IR) relations of the faint extragalactic radio sources is important for using radio emission as a tracer of star formation in high redshift (z) star-forming galaxies (SFGs). Using deep uGMRT observations of the ELAIS-N1 field in the 0.3-0.5 GHz range, we study the statistical properties of the radio-IR relations a…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 8
Seimei KOOLS-IFU mapping of the gas and dust distributions in Galactic planetary nebulae: the case of IC 2165
DOI: 10.1093/mnras/stac260 Bibcode: 2022MNRAS.511.4774O

Otsuka, Masaaki

We investigated the physical and chemical properties of the gas and dust components in a carbon-rich planetary nebula (PN) IC 2165 using two-dimensional emission-line maps with superior resolution. The extinction map is generated in a self-consistent and assumption-free manner. The circumstellar gas-to-dust mass ratio (GDR) map ranges radially fro…

2022 Monthly Notices of the Royal Astronomical Society
AKARI IUE eHST 8
Searching for the next Galactic Luminous red nova
DOI: 10.1093/mnras/stac2685 Bibcode: 2022MNRAS.517.1884A

Jones, David; Blagorodnova, Nadejda; Erasmus, Nicolas +3 more

Luminous red novae (LRNe) are astrophysical transients believed to be caused by the partial ejection of a binary star's common envelope (CE) and the merger of its components. The formation of the CE is likely to occur during unstable mass transfer, initiated by a primary star which is evolving off the main sequence (a Hertzsprung gap star) and a l…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era
DOI: 10.1093/mnras/stac1095 Bibcode: 2022MNRAS.513.2822G

Kovács, J.; Claret, A.; Kundra, E. +4 more

Rapidly rotating early-type main-sequence stars with transiting planets are interesting in many aspects. Unfortunately, several astrophysical effects in such systems are not well understood yet. Therefore, we performed a photometric mini-survey of three rapidly rotating stars with transiting planets, namely KELT-17b, KELT-19Ab, and KELT-21b, using…

2022 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 8
Stars in the local galactic thick disc and halo in Gaia EDR3: a catalogue of half a million local main-sequence stars with photometric metallicities
DOI: 10.1093/mnras/stab3671 Bibcode: 2022MNRAS.510.4308K

Kim, Bokyoung; Lépine, Sebastien

We present a catalogue of 551 214 main-sequence stars in the local (d < 2 kpc) Galactic thick disc and halo, based on a search of stars with large proper motions ($\mu _{\rm tot} \gt 40.0~\rm mas\, yr^{-1}$) in the Gaia Early Data Release 3. We derive photometric metallicity calibrated from the colour-luminosity-metallicity distribution of 20 0…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
The XMM Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
DOI: 10.1093/mnras/stac2463 Bibcode: 2022MNRAS.517..657T

Romer, A. K.; Mann, R. G.; Klein, M. +10 more

We present the first comparison between properties of clusters of galaxies detected by the eROSITA Final Equatorial-Depth Survey (eFEDS) and the XMM Cluster Survey (XCS). We have compared, in an ensemble fashion, properties from the eFEDS X-ray cluster catalogue with those from the Ultimate XMM eXtragaLactic (XXL) survey project (XXL-100-GC). We f…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 8
Search for OB associations in Gaia Early Data Release 3
DOI: 10.1093/mnras/stac1780 Bibcode: 2022MNRAS.515.4359C

de Grijs, Richard; Chemel, Alexander A.; Glushkova, Elena V. +1 more

The distribution of young stars into OB associations has long been in need of updating. High-precision Gaia Early Data Release 3 astrometry, coupled with modern machine-learning methods, allows this to be done. We have compiled a well-defined sample which includes OB stars and young open clusters (OCs), in total comprising about 47 700 objects. To…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
Pulsating subdwarf B stars in the oldest open cluster NGC 6791
DOI: 10.1093/mnras/stab2985 Bibcode: 2022MNRAS.509..763S

Reed, M. D.; Pelisoli, I.; Németh, P. +6 more

We report results of our analysis of the Kepler superaperture LC data of the open cluster NGC 6791 to search for pulsating sdB stars. We checked all pixels and we found only three sdB stars to be pulsating, KIC 2569576 (B3), KIC 2438324 (B4), and KIC 2437937 (B5). These stars were known to be pulsators before, though we extended data coverage dete…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
Detection of 125.5-day optical periodic modulation of the neutron star M51 ULX-8
DOI: 10.1093/mnras/stac2887 Bibcode: 2022MNRAS.517.3495A

Allak, S.

Studying Ultraluminous X-ray sources (ULXs) in the optical wavelengths provides important clues about the accretion mechanisms and the evolutionary processes of X-ray binary systems. In this study, three (C1, C2, and C3) possible optical counterparts were identified for well-known neutron star (NS) candidate M51 ULX-8 through advanced astrometry b…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 8