Search Results - "Dobrotka, Andrej"
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The RS Oph Outburst of 2021 Monitored in X-Rays with NICER
Published in The Astrophysical journal (01-09-2023)“…Abstract The 2021 outburst of the symbiotic recurrent nova RS Oph was monitored with the Neutron Star Interior Composition Explorer Mission (NICER) in the…”
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2
X-ray spectra and light curves of cooling novae and a nova like
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT We present X-ray observations of novae V2491 Cyg and KT Eri about 9 yr post-outburst of the dwarf nova and post-nova candidate EY Cyg, and of a VY Scl…”
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3
Nova LMC 2009a as observed with XMM–Newton, compared with other novae
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT We examine four high-resolution reflection grating spectrometers (RGS) spectra of the February 2009 outburst of the luminous recurrent nova LMC 2009a…”
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4
What We Learn from the X-Ray Grating Spectra of Nova SMC 2016
Published in The Astrophysical journal (01-08-2018)“…Nova SMC 2016 has been the most luminous nova known in the direction of the Magellanic Clouds. It turned into a very luminous supersoft X-ray source between…”
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5
All Quiet in Globular Clusters
Published in The Astrophysical journal (20-03-2006)“…Cataclysmic variables (CVs) should be present in large numbers in globular clusters (GCs). Numerous low-luminosity X-ray sources identified over the past few…”
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6
Deductions from the Indication of Eclipses of Nova V1493 Aql
Published in Astrophysics and space science (01-08-2006)“…Issue Title: Close Binaries in the 21st Century: New Opportunities and Challenges Our mainly R band photometry of V1493 Aql (1999) during its outburst,…”
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7
Shocks in the outflow of the RS Oph 2021 eruption observed with X-ray gratings
Published 05-09-2022“…The 2021 outburst of the symbiotic recurrent nova RS Oph was observed with the Chandra High Energy Transmission Gratings (HETG) on day 18 after optical maximum…”
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8
The RS Oph outburst of 2021 monitored in X-rays with NICER
Published 21-07-2023“…The 2021 outburst of the symbiotic recurrent nova RS Oph was monitored with the Neutron Star Interior Composition Explorer Mission (NICER) in the 0.2-12 keV…”
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9
X-ray Spectra and Light Curves of Cooling Novae and a Nova-Like
Published 29-09-2020“…We present X-ray observations of novae V2491 Cyg and KT Eri about 9 years post-outburst, of the dwarf nova and post-nova candidate EY Cyg, and of a VY Scl…”
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10
Nova LMC 2009a as observed with XMM-Newton, compared with other novae
Published 11-05-2021“…We examine four high resolution reflection grating spectrometers (RGS) spectra of the February 2009 outburst of the luminous recurrent nova LMC 2009a. They…”
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11
The supersoft X-ray transient ASASSN-16oh as a thermonuclear runaway without mass ejection
Published 30-06-2019“…The Astrophysical Journal Letters, Volume 879:L5 (5pp), 2019 The supersoft X-ray and optical transient ASASSN-16oh has been interpreted by Maccarone et al…”
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12
Multifrequency nature of the 0.75 mHz feature in the X-ray light curves of the nova V4743 Sgr
Published 11-03-2010“…We present timing analyses of eight X-ray light curves and one optical/UV light curve of the nova V4743 Sgr (2002) taken by CHANDRA and XMM on days after…”
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13
Flickering study of nova like systems KR Aur and UU Aqr
Published 16-11-2011“…We present a study of the flickering activity in two nova like systems KR Aur and UU Aqr. We applied a statistical model of flickering simulations in accretion…”
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14
V4745 Sgr -- a nova above the period gap and an intermediate polar candidate
Published 22-05-2006“…Mon.Not.Roy.Astron.Soc.371:459-464,2006 A period analysis of CCD unfiltered photometry of V4745 Sgr (Nova Sgr 2003 #1) performed during 23 nights in the years…”
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15
All Quiet in Globular Clusters
Published 13-09-2005“…Astrophys.J.640:288-298,2006 Cataclysmic Variables (CVs) should be present in large numbers in Globular Clusters (GCs). Numerous low-luminosity X-ray sources…”
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16
The possible orbital period of the nova V1493 Aquilae
Published 11-11-2005“…Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 no. 1) performed during 12 nights through I and R filters a few weeks after maximum is presented…”
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