Search Publications

Mid-infrared imaging of Supernova 1987A
DOI: 10.1093/mnras/stac3036 Bibcode: 2022MNRAS.517.4327M

Matsuura, Mikako; Barlow, M. J.; Meixner, Margaret +9 more

At a distance of 50 kpc, Supernova 1987A is an ideal target to study how a young supernova (SN) evolves in time. Its equatorial ring, filled with material expelled from the progenitor star about 20 000 yr ago, has been engulfed with SN blast waves. Shocks heat dust grains in the ring, emitting their energy at mid-infrared (IR) wavelengths We prese…

2022 Monthly Notices of the Royal Astronomical Society
eHST 7
The VMC survey - XLIX. Discovery of a population of quasars dominated by nuclear dust emission behind the Magellanic Clouds
DOI: 10.1093/mnras/stac2096 Bibcode: 2022MNRAS.515.6046P

Maitra, Chandreyee; Hopkins, Andrew M.; Haberl, Frank +14 more

Following the discovery of SAGE0536AGN (z ~ 0.14), with the strongest 10-µm silicate emission ever observed for an active galactic nucleus (AGN), we discovered SAGE0534AGN (z ~ 1.01), a similar AGN but with less extreme silicate emission. Both were originally mistaken as evolved stars in the Magellanic Clouds. Lack of far-infrared emission, …

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 7
SRG/eROSITA view of X-ray reflection in the Central Molecular Zone: a snapshot in September-October 2019
DOI: 10.1093/mnras/stab3333 Bibcode: 2022MNRAS.509.6068K

Khabibullin, Ildar; Churazov, Eugene; Sunyaev, Rashid

X-ray reflection off dense molecular clouds in the Galactic Centre region has established itself as a powerful probe for the past activity record of the supermassive black hole Sgr A* on a time-scale of a few hundred years. Detailed studies of the reflection signal from individual clouds allow us to estimate parameters of the brightest flare(s) an…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
Modelling multiwavelength emission of Ultra-luminous X-ray Sources accreting above the Eddington limit
DOI: 10.1093/mnras/stab3240 Bibcode: 2022MNRAS.509.4694A

Wolter, A.; Pintore, F.; Zampieri, L. +1 more

We model the multiwavelength properties of binaries accreting at super-critical rates with the aim to better understand the observational properties of Ultra-luminous X-ray Sources (ULXs). We calculate an extended grid of binary systems which evolve through Roche Lobe Overflow and undergo case A mass transfer from massive donors (up to 25 ${\rm M}…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
Trumpler 16-26: a new centrifugal magnetosphere star discovered via SDSS/APOGEE H-band spectroscopy
DOI: 10.1093/mnras/stac2396 Bibcode: 2022MNRAS.516.2812C

Rivinius, Thomas; Nidever, David L.; Labadie-Bartz, Jonathan +6 more

We report the discovery of a new example of the rare class of highly magnetized, rapidly rotating, helium enhanced, early B stars that produce anomalously wide hydrogen emission due to a centrifugal magnetosphere (CM). The star is Trumpler 16-26, a B1.5 V member of the Trumpler 16 open cluster. A CM was initially suspected based on hydrogen Bracke…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
The progenitor of the Vela pulsar
DOI: 10.1093/mnras/stac098 Bibcode: 2022MNRAS.511.3428K

Kochanek, C. S.

With Gaia parallaxes, it is possible to study the stellar populations associated with individual Galactic supernova remnants (SNRs) to estimate the mass of the exploding star. Here, we analyse the luminous stars near the Vela pulsar and SNR to find that its progenitor was probably ($\mathrel {\raise.3ex\rm{\gt }\lower0.6ex\rm{\sim }}90\rm \,per\,c…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Kinematics of luminous blue variables in the Large Magellanic Cloud
DOI: 10.1093/mnras/stac2265 Bibcode: 2022MNRAS.516.2142A

Choi, Yumi; Smith, Nathan; Andrews, Jennifer +3 more

We study the kinematics of luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC). Using high-resolution spectra, we measure the systemic radial velocities for a sample of 16 LBVs and LBV candidates. In order to measure the net motion of LBVs compared to their local environments, we subtract the projected line-of-sight velocity at the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
A detailed study of stellar populations of three star clusters with extended main-sequence turnoffs
DOI: 10.1093/mnras/stab3589 Bibcode: 2022MNRAS.512.3992C

Li, Zhongmu; Chen, Jing; Zhang, Su +2 more

This paper investigates the extended main-sequence turnoffs (eMSTOs) and stellar populations of three clusters with different ages using Gaia Data Release 2 (DR2) data in detail. The colour-magnitude diagrams (CMDs) of three Galactic clusters show broad main sequences, eMSTOs, blue stragglers, and red giant clumps. We explore the effects of age sp…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Multiple giant eruptions and X-ray emission in the recoiling AGN/LBV candidate SDSS1133
DOI: 10.1093/mnras/stac1685 Bibcode: 2022MNRAS.515..110K

Kokubo, Mitsuru

We present a comprehensive analysis of 20 yr worth of multicolour photometric light curves, multiepoch optical spectra, and X-ray data of an off-nuclear variable object SDSS1133 in Mrk 177 at z = 0.0079. The UV-optical light curves reveal that SDSS1133 experienced four outbursts in 2001, 2014, 2019, and 2021. The persistent UV-optical luminosity i…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 7
Collimation of the kiloparsec-scale radio jets in NGC 2663
DOI: 10.1093/mnras/stac2012 Bibcode: 2022MNRAS.516.1865V

Salvato, M.; Nandra, K.; Filipović, M. D. +25 more

We present the discovery of highly collimated radio jets spanning a total of 355 kpc around the nearby elliptical galaxy NGC 2663, and the possible first detection of recollimation on kiloparsec scales. The small distance to the galaxy (~28.5 Mpc) allows us to resolve portions of the jets to examine their structure. We combine multiwavelength data…

2022 Monthly Notices of the Royal Astronomical Society
eHST 7