Search Publications

Gaia view of a stellar sub-structure in front of the Small Magellanic Cloud
DOI: 10.1093/mnras/staa3085 Bibcode: 2021MNRAS.500.2757O

de Grijs, Richard; Cioni, Maria-Rosa L.; Bekki, Kenji +6 more

Recent observational studies identified a foreground stellar sub-structure traced by red clump (RC) stars (∼12 kpc in front of the main body) in the eastern regions of the Small Magellanic Cloud (SMC) and suggested that it formed during the formation of the Magellanic Bridge (MB), due to the tidal interaction of the Magellanic Clouds. Previous stu…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
LAMOST J0140355 + 392651: an evolved cataclysmic variable donor transitioning to become an extremely low-mass white dwarf
DOI: 10.1093/mnras/stab1318 Bibcode: 2021MNRAS.505.2051E

Xiang, Maosheng; Rix, Hans-Walter; El-Badry, Kareem +6 more

We present LAMOST J0140355 + 392651 (hereafter J0140), a close (Porb = 3.81 h) binary containing a bloated, low-mass ($M \approx 0.15 \, \mathrm{M}_{\odot }$) proto-white dwarf (WD) and a massive ($M \approx 0.95\, \mathrm{M}_{\odot }$) WD companion. The system's optical light curve is dominated by large-amplitude ellipsoidal variabilit…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
The age of the carina young association and potential membership of HD 95086
DOI: 10.1093/mnras/staa3631 Bibcode: 2021MNRAS.500.5552B

Booth, Mark; del Burgo, Carlos; Hambaryan, Valeri V.

Carina is a nearby young stellar association. So far, only a small number of stars have been clearly identified as members of this association. In this paper, we reanalyse the membership of the association in light of Gaia DR2 data, in particular finding that HD 95086 is a potential member (probability of 71 per cent). This star is noteworthy as o…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
Photometric, polarimetric, and spectroscopic studies of the luminous, slow-decaying Type Ib SN 2012au
DOI: 10.1093/mnras/stab1889 Bibcode: 2021MNRAS.507.1229P

Pandey, S. B.; Ochner, P.; Benetti, S. +15 more

Optical, near-infrared (NIR) photometric and spectroscopic studies, along with the optical imaging polarimetric results for SN 2012au, are presented in this article to constrain the nature of the progenitor and other properties. Well-calibrated multiband optical photometric data (from -0.2 to +413 d since B-band maximum) were used to compute the b…

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
Detailed elemental abundances of binary stars: searching for signatures of planet formation and atomic diffusion
DOI: 10.1093/mnras/stab2471 Bibcode: 2021MNRAS.508.1227L

Bitsch, Bertram; Ting, Yuan-Sen; Murphy, Michael T. +5 more

Binary star systems are assumed to be co-natal and coeval, and thus to have identical chemical composition. In this work, we aim to test the hypothesis that there is a connection between observed element abundance patterns and the formation of planets using binary stars. Moreover, we also want to test how atomic diffusion might influence the obser…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
Internal rotation of Milky Way dwarf spheroidal satellites with Gaia Early Data Release 3
DOI: 10.1093/mnras/stab1568 Bibcode: 2021MNRAS.505.5884M

van der Marel, Roeland P.; Watkins, Laura L.; del Pino, Andrés +2 more

We present an analysis of the kinematics of 14 satellites of the Milky Way (MW). We use proper motions (PMs) from the Gaia Early Data Release 3 (EDR3) and line-of-sight velocities (vlos) available in the literature to derive the systemic 3D motion of these systems. For six of them, namely the Carina, Draco, Fornax, Sculptor, Sextans, an…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 24
Revealing the formation histories of the first stars with the cosmic near-infrared background
DOI: 10.1093/mnras/stab2697 Bibcode: 2021MNRAS.508.1954S

Furlanetto, Steven R.; Sun, Guochao; Mirocha, Jordan +1 more

The cosmic near-infrared background (NIRB) offers a powerful integral probe of radiative processes at different cosmic epochs, including the pre-reionization era when metal-free, Population III (Pop III) stars first formed. While the radiation from metal-enriched, Population II (Pop II) stars likely dominates the contribution to the observed NIRB …

2021 Monthly Notices of the Royal Astronomical Society
eHST 24
Fundamental X-ray corona parameters of Swift/BAT AGN
DOI: 10.1093/mnras/stab1976 Bibcode: 2021MNRAS.506.4960H

Mushotzky, Richard; Hinkle, Jason T.

While X-ray emission from active galactic nuclei (AGN) is common, the detailed physics behind this emission is not well understood. This is in part because high quality broad-band spectra are required to precisely derive fundamental parameters of X-ray emission, such as the photon index, folding energy, and reflection coefficient. Here, we present…

2021 Monthly Notices of the Royal Astronomical Society
XMM-Newton 24
Photometric cross-calibration of the SDSS Stripe 82 Standard Stars catalogue with Gaia EDR3, and comparison with Pan-STARRS1, DES, CFIS, and GALEX catalogues
DOI: 10.1093/mnras/stab1452 Bibcode: 2021MNRAS.505.5941T

Gwyn, Stephen; Ivezić, Željko; Tucker, Douglas L. +3 more

We extend the SDSS Stripe 82 Standard Stars catalogue with post-2007 SDSS imaging data. This improved version lists averaged SDSS ugriz photometry for nearly a million stars brighter than r ~ 22 mag. With 2-3 times more measurements per star, random errors are 1.4-1.7 times smaller than in the original catalogue, and about three times smaller than…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 24
Signature of the turbulent component of the solar dynamo on active region scales and its association with flaring activity
DOI: 10.1093/mnras/stab2404 Bibcode: 2021MNRAS.507.3698A

Abramenko, Valentina I.

It is a challenging problem to obtain observational evidence of the turbulent component of solar dynamo operating in the convective zone because the dynamo action is hidden below the photosphere. Here we present results of a statistical study of flaring active regions (ARs) that produced strong solar flares of an X-ray class X1.0 and higher during…

2021 Monthly Notices of the Royal Astronomical Society
SOHO 24