Search Publications

Are magnetic fields universal in O-type multiple systems?
DOI: 10.1093/mnras/stad730 Bibcode: 2023MNRAS.521.6228H

Ilyin, I.; Hubrig, S.; Schöller, M. +2 more

Although significant progress has been achieved in recent surveys of the magnetism in massive stars, the origin of the detected magnetic fields remains to be the least understood topic in their studies. We present an analysis of 61 high-resolution spectropolarimetric observations of 36 systems with O-type primaries, among them 10 known particle-ac…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
The EBLM project X. Benchmark masses, radii, and temperatures for two fully convective M-dwarfs using K2
DOI: 10.1093/mnras/stad452 Bibcode: 2023MNRAS.521.6305D

Hellier, Coel; Triaud, Amaury H. M. J.; Sairam, Lalitha +23 more

M-dwarfs are the most abundant stars in the galaxy and popular targets for exoplanet searches. However, their intrinsic faintness and complex spectra inhibit precise characterization. We only know of dozens of M-dwarfs with fundamental parameters of mass, radius, and effective temperature characterized to better than a few per cent. Eclipsing bina…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Optical and X-ray studies of Be/X-ray binary 1A 0535+262 during its 2020 giant outburst
DOI: 10.1093/mnras/stac3354 Bibcode: 2023MNRAS.518.5089C

Naik, Sachindra; Jana, Arghajit; Jaisawal, Gaurava K. +3 more

We report results obtained from the optical and X-ray studies of the Be/X-ray binary 1A 0535+262/HD 245770 during the 2020 October giant X-ray outburst, using the 1.2-m telescope at Mount Abu Infrared observatory and AstroSat, respectively. The peak flux of the outburst was recorded to be ~11 Crab in the 15-50 keV range, the highest ever observed …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
An excursion into the core of the cluster lens Abell 1689
DOI: 10.1093/mnras/stad2418 Bibcode: 2023MNRAS.525.2519G

Scarlata, Claudia; Liesenborgs, Jori; Alavi, Anahita +3 more

Abell 1689 is a well-studied cluster of galaxies and one of the largest gravitational lens systems ever observed. We have obtained a reconstruction of the cluster Abell 1689 using GRALE, a free-form lens inversion method that relies exclusively on the multiple image data. Non-inclusion of any data related to cluster member galaxies ensures an unbi…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
Discovery of delta Scuti variables in eclipsing binary systems II. Southern TESS field search
DOI: 10.1093/mnras/stad1898 Bibcode: 2023MNRAS.524..619K

Kahraman Aliçavuş, F.; Aliçavuş, F.; Çoban, Ç. G. +3 more

The presence of pulsating stars in eclipsing binary systems (EBs) makes these objects significant since they allow us to investigate the stellar interior structure and evolution. Different types of pulsating stars could be found in EBs, such as δ Scuti variables. δ Scuti stars in EBs have been known for decades, and the increasing number of such s…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Spectroscopic follow-up of statistically selected extremely metal-poor star candidates from GALAH DR3
DOI: 10.1093/mnras/stad170 Bibcode: 2023MNRAS.520..917D

Spitler, Lee R.; Da Costa, G. S.; Buder, Sven +5 more

The advent of large-scale stellar spectroscopic surveys naturally leads to the implementation of machine learning techniques to isolate, for example, small sub-samples of potentially interesting stars from the full data set. A recent example is the application of the t-SNE statistical method to ~600 000 stellar spectra from the GALAH survey in ord…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Accelerated phase-mixing in the stellar halo due to a rotating bar
DOI: 10.1093/mnrasl/slad017 Bibcode: 2023MNRAS.521L..24D

Vasiliev, Eugene; Belokurov, Vasily; Davies, Elliot Y. +1 more

In a galaxy merger, the stars tidally stripped from the satellite and accreted onto the host galaxy undergo phase-mixing and form finely grained structures in the phase space. However, these fragile structures may be destroyed in the subsequent galaxy evolution, in particular, by a rotating bar that appears well after the merger is completed. In t…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Multiwavelength study of NGC 1365: The obscured active nucleus and off-nuclear compact X-ray sources
DOI: 10.1093/mnras/stad337 Bibcode: 2023MNRAS.520.3712S

Shalima, P.; Swain, Subhashree; Dewangan, Gulab Chand +2 more

We present a multiwavelength study of the active nucleus and the off-nuclear X-ray sources in the nearby spiral galaxy, NGC 1365 using three simultaneous UV/X-ray observations by AstroSat over a two months period and archival IR observations performed with Spitzer and Herschel. Utilizing the data from the Soft X-ray Telescope (SXT) onboard AstroSa…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 9
New stellar velocity substructures from Gaia DR3 proper motions
DOI: 10.1093/mnras/stac3649 Bibcode: 2023MNRAS.519.1989M

McMillan, Paul J.; Hobbs, David; Mikkola, Daniel

Local stellar motions are expected, and have been shown, to include signatures of the Galaxy's past dynamical evolution. These are typically divided into the disc, which shows the dynamical effects of spiral arms and the bar, and the stellar halo, with structures thought to be debris from past mergers. We use Gaia Data Release 3 to select large sa…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Reconstructing the genesis of a globular cluster system at a look-back time of 9.1 Gyr with the JWST
DOI: 10.1093/mnrasl/slac162 Bibcode: 2023MNRAS.520L..58F

Forbes, Duncan A.; Romanowsky, Aaron J.

Using early-release data from the JWST, Mowla et al. and Claeyssens et al. recently measured various properties for gravitationally lensed compact sources ('sparkles') around the 'Sparkler' galaxy at a redshift of 1.378 (a look-back time of 9.1 Gyr). Here, we focus on the Mowla et al. as they were able to break the age-metallicity degeneracy and d…

2023 Monthly Notices of the Royal Astronomical Society
JWST 8