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A broad-band X-ray study of the asynchronous polar CD Ind
DOI: 10.1093/mnras/stac296 Bibcode: 2022MNRAS.511.4981D

Dutta, Anirban; Rana, Vikram

We present a simultaneous broad-band analysis of X-ray data obtained with the XMM-Newton and the Nuclear Spectroscopic Telescope Array (NuSTAR) for the asynchronous polar source, CD Ind. The spin-folded light curve in the soft 0.3-3.0 keV band shows a single broad hump-like structure superimposed with occasional narrow dips, indicating a single-po…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
Discovery of a highly eccentric, chromospherically active binary: ASASSN-V J192114.84+624950.8
DOI: 10.1093/mnras/stac1343 Bibcode: 2022MNRAS.514..200W

Kochanek, C. S.; Holoien, Thomas W. -S.; Stanek, K. Z. +5 more

As part of an All-Sky Automated Survey for SuperNovae (ASAS-SN) search for sources with large flux decrements, we discovered a transient where the quiescent, stellar source ASASSN-V J192114.84+624950.8 rapidly decreased in flux by $\sim 55{{\ \rm per\ cent}}$ (~0.9 mag) in the g band. The Transiting Exoplanet Survey Satellite light curve revealed …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Statistical properties of cataclysmic variables in the local galactic disc: a joint analysis of Gaia and XMM-Newton data
DOI: 10.1093/mnras/stac2354 Bibcode: 2022MNRAS.516.1263X

Wang, Q. Daniel; Xu, Xiao-jie; Li, Xiangdong

Cataclysmic variables (CVs) represent a key evolutionary phase of many low-mass stellar binaries and appear to collectively dominate the galactic X-ray background above ~1 keV. Statistical properties of CVs, however, remain poorly understood, even in the solar neighbourhood. We aim to obtain an X-ray luminosity-complete sample of local CVs whose d…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
Herschel discovery of far-infrared emission from the hotspot D in the radio galaxy Cygnus A
DOI: 10.1093/mnras/stac826 Bibcode: 2022MNRAS.512.5995S

Isobe, Naoki; Tashiro, Makoto S.; Sunada, Yuji +3 more

The far-infrared counterpart of hotspot D, the terminal hotspot of the eastern jet hosted by the radio galaxy Cygnus A, is detected with Herschel Aperture photometry of the source performed in 5 photometric bands covering the wavelength range of 70-350 $\mu$m. After removing the contamination from another nearby hotspot, E, the far-infrared intens…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 3
Fast prograde coronal flows in solar active regions
DOI: 10.1093/mnrasl/slac079 Bibcode: 2022MNRAS.515L..84H

Chamberlin, Phillip C.; Fletcher, Lyndsay; Mulay, Sargam M. +6 more

We report the discovery and characterization of high-speed (>100 km s-1) horizontal flows in solar active regions, making use of the Sun-as-a-star spectroscopy in the range 5-105 nm provided by the EVE (Extreme Ultraviolet Variability Experiment) spectrometers on the Solar Dynamics Observatory. These apparent flows are persistent on …

2022 Monthly Notices of the Royal Astronomical Society
Hinode 3
Chandra revisits WR 48a: testing colliding wind models in massive binaries
DOI: 10.1093/mnras/stab3469 Bibcode: 2022MNRAS.510.1278Z

Skinner, Stephen L.; Zhekov, Svetozar A.; Gagné, Marc

We present results of new Chandra High-Energy Transmission Grating (HETG) observations (2019 November-December) of the massive Wolf-Rayet binary WR 48a. Analysis of these high-quality data showed that the spectral lines in this massive binary are broadened (full width at half-maximum, FWHM = 1400 km s-1) and marginally blueshifted (~-10…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
Unravelling the nature of the dual AGN in the galaxy pair system IRAS 05589+2828 and 2MASX J06021107 + 2828382
DOI: 10.1093/mnras/stac2244 Bibcode: 2022MNRAS.516.5270B

Jiménez-Bailón, E.; Marziani, P.; Chavushyan, V. H. +10 more

We have studied the nuclear region of the previously detected dual AGN system in the galaxy pair IRAS 05589 + 2828 and 2MASX J06021107 + 2828382, through new optical spectroscopy observations, along with radio and X-ray archival data. Our multiwavelength data strongly suggest that the Sy1 IRAS 05589+2828 (z = 0.0330 ± 0.0002) conforms to a dual AG…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 3
Spiral density-wave structure parameters in the solar neighbourhood derived from longitudinal velocities of Gaia EDR3 OB stars: 3D approach
DOI: 10.1093/mnras/stab2971 Bibcode: 2022MNRAS.509..463G

Mróz, Przemek; Gedalin, Michael; Jiang, Ing-Guey +2 more

Distances and transverse along the Galactic longitude velocities vl of 2640 Gaia EDR3 O-B2 stars of Xu et al. within 2.5 kpc from the Sun and 250 pc from the Galactic plane with relative distance and velocity accuracies of <10 and <50 per cent are selected. Under the assumption of spiral density waves, both Galactic differential r…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories
DOI: 10.1093/mnras/stac2696 Bibcode: 2022MNRAS.517.3312M

Galbany, L.; Mollá, M.; Gomes, J. M. +5 more

We present a summary of our project that studies galaxies hosting type Ia supernova (SN Ia) at different redshifts. We present Gran Telescopio de Canarias (GTC) optical spectroscopy of six SN Ia host galaxies at redshift z ~ 0.4-0.5. They are joined to a set of SN Ia host galaxies at intermediate-high redshift, which include galaxies from surveys …

2022 Monthly Notices of the Royal Astronomical Society
eHST 3
Probing the parameters of the intergalactic medium using quasars
DOI: 10.1093/mnras/stac814 Bibcode: 2022MNRAS.513..822D

Morris, Simon L.; Fumagalli, Michele; Gatuzz, Efrain +1 more

We continue our series of papers on intergalactic medium (IGM) tracers using quasi-stellar objects (QSOs), having examined gamma-ray bursts (GRBs) and blazars in earlier studies. We have estimated the IGM properties of hydrogen column density ($\mathit {N}\small {\rm HXIGM}$), temperature, and metallicity using XMM-Newton QSO spectra over a large …

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 3