Search Results - "Stoyanov, K. A."
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Rotational velocities of the giants in symbiotic stars – III. Evidence of fast rotation in S-type symbiotics
Published in Monthly notices of the Royal Astronomical Society (11-10-2008)“…We have measured the projected rotational velocities (v sin i) in a number of symbiotic stars and M giants using high-resolution spectroscopic observations. On…”
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Orbital parameters of the high-mass X-ray binary 4U 2206+54
Published in Astronomische Nachrichten (01-12-2014)“…We present new radial velocities of the high‐mass X‐ray binary star 4U 2206+54 based on optical spectra obtained with the Coudé spectrograph at the 2 m RCC…”
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Difference between the optical flickering colours of cataclysmic variables and symbiotic recurrent novae
Published in Astronomische Nachrichten (01-03-2015)“…We performed simultaneous observations in 3 bands (U BV) of the flickering variability of the recurrent novae RS Oph and T CrB at quiescence. Using new and…”
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AG Pegasi – now a classical symbiotic star in outburst?
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)“…Optical spectroscopy study of the recent AG Pegasi (AG Peg) outburst observed during the second half of 2015 is presented. Considerable variations of the…”
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UBVRI observations of the flickering of RS Ophiuchi at quiescence
Published in Monthly notices of the Royal Astronomical Society (01-05-2010)“…We report observations of the flickering variability of the recurrent nova RS Oph at quiescence on the basis of simultaneous observations in five bands…”
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The origin of the high-mass X-ray binary 4U 2206+54/BD+532790
Published in Monthly notices of the Royal Astronomical Society (23-02-2022)“…ABSTRACT Based on the Gaia EDR3 astrometric parameters and our new systemic radial velocity of the high-mass X-ray binary 4U 2206+54/BD+532790, we studied the…”
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An eccentric wave in the circumstellar disc of the Be/X-ray binary X Persei
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT We present spectroscopic observations of the Be/X-ray binary X Per obtained during the period 2017 December–2020 January (MJD 58095–58865). In 2017…”
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Size of the accretion disc in the recurrent nova T CrB
Published in Astronomische Nachrichten (01-07-2024)“…Abstract We present high‐resolution (0.06 Å px) spectroscopic observations of the recurrent nova T Coronae Borealis obtained during the last 1.5 years…”
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Optical Spectroscopy and X-Ray Observations of the D-Type Symbiotic Star EF Aql
Published in Monthly notices of the Royal Astronomical Society (11-06-2020)“…We performed high-resolution optical spectroscopy and X-ray observations of the recently identified Mira-type symbiotic star EF Aql. Based on high-resolution…”
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Flickering of the jet‐ejecting symbiotic star MWC 560
Published in Astronomische Nachrichten (01-05-2020)“…We analyzed the optical photometric data of short‐term variability (flickering) of the accreting white dwarf in the jet‐ejecting symbiotic star MWC 560. The…”
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Flickering of accreting white dwarfs: the remarkable amplitude–flux relation and disc viscosity
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2016)“…We analyse optical photometric data of short term variability (flickering) of accreting white dwarfs in cataclysmic variables (KR Aur, MV Lyr, V794 Aql, TT…”
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Discovery of optical flickering from the symbiotic star EF Aquilae
Published in Astronomische Nachrichten (01-07-2017)“…We report optical charge‐coupled device (CCD) photometry of the recently identified symbiotic star EF Aquilae (EF Aql). Our observations in the Johnson V and B…”
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The cataclysmic variable AE Aquarii: B–V color of the flares
Published in Astronomische Nachrichten (01-06-2017)“…We report simultaneous observations of the flaring behavior of the cataclysmic variable star AE Aquarii (AE Aqr). The observations are in Johnson B and V…”
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AG Pegasi – now a classical symbiotic star in outburst?
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)Get full text
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Transient and asymmetric dust structures in the TeV-bright nova RS Oph revealed by spectropolarimetry
Published 20-09-2023“…A&A 679, A150 (2023) A long-standing question related to nova eruptions is how these eruptions can lead to the formation of dust despite the ostensibly…”
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Optical spectroscopy of Be stars: peak separation of Balmer emission lines
Published 23-02-2023“…The Be stars display variable optical emission lines originating in the circumstellar disc. Here we analyse high resolution spectroscopic observations of Be…”
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The origin of the high-mass X-ray binary 4U 2206+54/BD +53 2790
Published 19-01-2022“…Based on the Gaia EDR3 astrometric parameters and our new systemic radial velocity of the high-mass X-ray binary 4U 2206+54/BD+53 2790, we studied the trace…”
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DSC study of thermal decomposition of partially ozonized diene rubbers
Published in Journal of applied polymer science (25-07-1996)“…The thermal decompositions of partially ozonized 1,4‐cis‐polybutadiene (E‐BR), 1,4‐cis‐polyisoprene (E‐IR), 1,4‐trans‐polyisoprene (Z‐IR),…”
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Simultaneous UBVRI observations of the cataclysmic variable AE Aquarii: Temperatures and masses of fireballs
Published in Astronomische Nachrichten (01-10-2012)“…We report simultaneous multicolour observations in 5 bands (UBVRI) of the flickering variability of the cataclysmic variable AE Aqr. Our aim is to estimate the…”
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Mass outflow from the symbiotic binary RS Oph during its 2021 outburst
Published 17-01-2023“…A&A 671, A49 (2023) RS Oph is a symbiotic recurrent nova containing a massive white dwarf with heavy mass loss during activity. In August 2021, it underwent…”
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