Search Publications

Inferring the morphology of AGN torus using X-ray spectra: a reliability study
DOI: 10.1093/mnras/stab3250 Bibcode: 2022MNRAS.509.5485S

Markowitz, Alex G.; Buchner, Johannes; Saha, Tathagata

Numerous X-ray spectral models have been developed to model emission reprocessed by the torus of an active galactic nucleus (AGN), e.g. UXCLUMPY, CTORUS, and MYTORUS. They span a range of assumed torus geometries and morphologies - some posit smooth gas distributions, and others posit distributions of clouds. It is suspected that given the quality…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
High-precision star-formation efficiency measurements in nearby clouds
DOI: 10.1093/mnras/stac174 Bibcode: 2022MNRAS.511.1431H

Gutermuth, Robert A.; Pokhrel, Riwaj; Hu, Zipeng +1 more

On average molecular clouds convert only a small fraction ϵff of their mass into stars per free-fall time, but different star-formation theories make contrasting claims for how this low mean efficiency is achieved. To test these theories, we need precise measurements of both the mean value and the scatter of ϵff, but high-pre…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 16
LeMMINGs - IV. The X-ray properties of a statistically complete sample of the nuclei in active and inactive galaxies from the Palomar sample
DOI: 10.1093/mnras/stab3310 Bibcode: 2022MNRAS.510.4909W

Muxlow, T. W. B.; Argo, M. K.; Knapen, J. H. +22 more

All 280 of the statistically complete Palomar sample of nearby (<120 Mpc) galaxies δ > 20° have been observed at 1.5 GHz as part of the LeMMINGs e-MERLIN legacy survey. Here, we present Chandra X-ray observations of the nuclei of 213 of these galaxies, including a statistically complete sub-set of 113 galaxies in the declination range 40° &l…

2022 Monthly Notices of the Royal Astronomical Society
eHST 16
CoBiToM Project - II. Evolution of contact binary systems close to the orbital period cut-off
DOI: 10.1093/mnras/stab3424 Bibcode: 2022MNRAS.514.5528L

Hatzidimitriou, D.; Hakala, P.; Liakos, A. +7 more

Ultra-short orbital period contact binaries (Porb < 0.26 d) host some of the smallest and least massive stars. These systems are faint and rare, and it is believed that they have reached a contact configuration after several Gyrs of evolution via angular momentum loss, mass transfer, and mass loss through stellar wind processes. This…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
UOCS -VIII. UV study of the open cluster NGC 2506 using ASTROSAT★
DOI: 10.1093/mnras/stac2421 Bibcode: 2022MNRAS.516.5318P

Subramaniam, Annapurni; Panthi, Anju; Vaidya, Kaushar +4 more

We study an intermediate-age open cluster (OC) NGC 2506 using the ASTROSAT/UVIT data and other archival data. We identified 2175 cluster members using a machine learning-based algorithm, ML-MOC, on Gaia EDR3 data. Among the cluster members detected in UVIT filters, F148W, F154W, and F169M, we detect nine blue straggler stars (BSS), three yellow st…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
Hard-X-ray-selected active galactic nuclei - II. Spectral energy distributions in the 5-45 GHz domain
DOI: 10.1093/mnras/stac1745 Bibcode: 2022MNRAS.515..473P

Laor, Ari; Behar, Ehud; Baldi, Ranieri D. +7 more

A wide-frequency radio study of active galactic nuclei (AGN) is crucial to evaluate the intervening radiative mechanisms responsible for the observed emission and relate them with the underlying accretion physics. We present wide-frequency (5-45 GHz), high-sensitivity (few $\mathrm{{\mu }Jy\, beam^{-1}}$), (sub)-kpc Jansky Very Large Array (JVLA) …

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 16
The white dwarf binary pathways survey - VII. Evidence for a bi-modal distribution of post-mass transfer systems?
DOI: 10.1093/mnras/stac673 Bibcode: 2022MNRAS.512.2625L

Gänsicke, B. T.; Parsons, S. G.; Hernandez, M. S. +5 more

Binary systems consisting of a white dwarf (WD) and a main-sequence companion with orbital periods up to ≈100 d are often thought to be formed through common envelope evolution which is still poorly understood. To provide new observational constraints on the physical processes involved in the formation of these objects, we are conducting a large-s…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 16
Von Zeipel - Lidov - Kozai cycles in action: Kepler triples with eclipse depth variations: KICs 6964043, 5653126, 5731312, and 8023317
DOI: 10.1093/mnras/stac1983 Bibcode: 2022MNRAS.515.3773B

Mitnyan, T.; Moe, M.; Toonen, S. +3 more

We report the results of the photodynamical analyses of four compact, tight triple stellar systems, KICs 6964043, 5653126, 5731312, and 8023317, based largely on Kepler and TESS data. All systems display remarkable eclipse timing and eclipse depth variations, the latter implying a non-aligned outer orbit. Moreover, KIC 6964043 is also a triply ecl…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
The post-common-envelope binary central star of the planetary nebula Ou 5: a doubly eclipsing post-red-giant-branch system
DOI: 10.1093/mnras/stab3736 Bibcode: 2022MNRAS.510.3102J

Corradi, Romano L. M.; Parsons, Steven G.; Munday, James +10 more

We present a detailed study of the stellar and orbital parameters of the post-common envelope binary central star of the planetary nebula Ou 5. Low-resolution spectra obtained during the primary eclipse - to our knowledge the first isolated spectra of the companion to a post-common-envelope planetary nebula central star - were compared to catalogu…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 16
The VMC survey - XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
DOI: 10.1093/mnras/stac712 Bibcode: 2022MNRAS.512.5423N

de Grijs, Richard; Ripepi, Vincenzo; Cioni, Maria-Rosa L. +7 more

We present proper motion (PM) measurements within the central region of the Large Magellanic Cloud (LMC), using near-infrared data from the VISTA survey of the Magellanic Cloud system (VMC). This work encompasses 18 VMC tiles covering a total sky area of ~28 deg2. We computed absolute stellar PMs from multiepoch observations in the K

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15