Search Publications

Hierarchical structure of YSO clusters in the W40 and Serpens South region: group extraction and comparison with fractal clusters
DOI: 10.1093/mnras/stac2362 Bibcode: 2022MNRAS.516.5258S

Wang, Hongchi; Gutermuth, Robert A.; Zhang, Shuinai +2 more

Young stellar clusters are believed to inherit the spatial distribution like hierarchical structures of their natal molecular cloud during their formation. However, the change of the structures between the cloud and the young clusters is not well constrained observationally. We select the W40-Serpens South region (~7 × 9 pc2) of the Aqu…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 5
Distances, extinctions, and stellar parameters for stars in SkyMapper DR3
DOI: 10.1093/mnras/stab3326 Bibcode: 2022MNRAS.510..433L

Lin, Jane; Casagrande, Luca; Asplund, Martin

We present a Bayesian isochrone fitting machinery to derive distances, extinctions, and stellar parameters (Teff, log g, and $\rm [Fe/H]$) for stars in the SkyMapper data release 3 (DR3) survey. We complement the latter with photometry from Gaia, 2MASS, and AllWISE, in addition to priors on parallaxes and interstellar extinction. We fin…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
A multi-instrument investigation of the frequency stability of oscillations above the acoustic cut-off frequency with solar activity
DOI: 10.1093/mnras/stac647 Bibcode: 2022MNRAS.512.5743K

Broomhall, A. -M.; Kiefer, R.; Kosak, K.

Below the acoustic cut-off frequency, oscillations are trapped within the solar interior and become resonant. However, signatures of oscillations persist above the acoustic cut-off frequency, and these travelling waves are known as pseudo-modes. Acoustic oscillation frequencies are known to be correlated with the solar cycle, but the pseudo-mode f…

2022 Monthly Notices of the Royal Astronomical Society
SOHO 5
IGR J18249-3243: a new GeV-emitting FR II and the emerging population of high-energy radio galaxies
DOI: 10.1093/mnras/stac865 Bibcode: 2022MNRAS.513..886B

Ricci, R.; Wieringa, M. H.; Giroletti, M. +10 more

The advent of new all-sky radio surveys such as the VLA Sky Survey and the Rapid ASKAP Continuum Survey, performed with the latest generation radio telescopes, is opening new possibilities on the classification and study of extragalactic γ-ray sources, specially the underrepresented ones like radio galaxies. In particular, the enhanced sensitivity…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 5
Transient two-pole accretion in the polar V496 UMa
DOI: 10.1093/mnras/stac885 Bibcode: 2022MNRAS.513.2930K

Garnavich, P. M.; Kennedy, M. R.; Littlefield, C.

We report XMM-Newton and TESS observations of V496 UMa, an AM Herculis-type cataclysmic variable. The XMM-Newton observation reveals that at times, two poles on the white dwarf accrete simultaneously, but accretion on to the secondary magnetic pole is erratic and can nearly cease in less than one binary orbit (1.5 h). Modelling of the X-ray spectr…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 5
Impacts of zonal winds on planetary oscillations and Saturn ring seismology
DOI: 10.1093/mnras/stac1957 Bibcode: 2022MNRAS.516..358D

Fuller, Jim; Dewberry, Janosz W.; Mankovich, Christopher R.

The excitation of density and bending waves in Saturn's C ring by planetary oscillation modes presents a unique opportunity to learn about gas giant interiors and rotation. However, theoretical complications related to Saturn's rapid and differential rotation pose a barrier to the full utilization of ring wave detections. We calculate oscillation …

2022 Monthly Notices of the Royal Astronomical Society
Cassini 5
Fundamental effective temperature measurements for eclipsing binary stars - II. The detached F-type eclipsing binary CPD-54 810
DOI: 10.1093/mnras/stac2968 Bibcode: 2022MNRAS.517.5129M

Maxted, P. F. L.; Southworth, J.; Tan, T. G. +2 more

CPD-54 810 is a double-lined detached eclipsing binary containing two mid-F type dwarfs on an eccentric 26-d orbit. We perform a combined analysis of the extensive photometry obtained by the TESS space mission along with previously published observations to obtain a full orbital and physical solution for the system. We measure the following model-…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
The XXL Survey - XLVIII. X-ray follow-up of distant XXL clusters: masses, scaling relations, and AGN contamination
DOI: 10.1093/mnras/stac617 Bibcode: 2022MNRAS.512.2525D

Valtchanov, I.; Pierre, M.; Gastaldello, F. +11 more

We use deep follow-up XMM-Newton observations of six clusters discovered in the XXL Survey at z > 1 to gain robust measurements of their X-ray properties and to investigate the extent to which scaling relations at low redshift are valid at z > 1. This sample is unique as it has been investigated for active galactic nucleus (AGN) contaminatio…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
The relation between X-ray and ultraviolet variability of quasars
DOI: 10.1093/mnras/stac738 Bibcode: 2022MNRAS.512.5511S

Xie, Zhang-Liang; Cai, Zhen-Yi; Wang, Jun-Xian +2 more

The relation between X-ray and UV/optical variability in AGNs has been explored in many individual sources, however a large sample study is yet absent. Through matching the XMM-Newton serendipitous X-ray and UV source catalogs with SDSS quasars, we build a sample of 802 epoch-pairs of 525 quasars showing clear variability in logFX - log…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
Spectroscopy of an extreme [O III] emitting active galactic nucleus at z = 3.212: implications for the reionization era
DOI: 10.1093/mnras/stab3279 Bibcode: 2022MNRAS.509.3102T

Feltre, Anna; Charlot, Stéphane; Shapley, Alice E. +4 more

Reionization-era galaxies often display intense nebular emission lines, both in rest-frame optical ([O III] + H β) and ultraviolet (UV; C III], C IV). How such strong nebular emission is powered remains unclear, with both active galactic nuclei (AGNs) and hot stars considered equally viable. The UV continuum slopes of these early systems tend to b…

2022 Monthly Notices of the Royal Astronomical Society
eHST 5