Search Results - "Kaminsky, B. M."
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Improved HCN/HNC linelist, model atmospheres and synthetic spectra for WZ Cas
Published in Monthly notices of the Royal Astronomical Society (01-03-2006)“…We build an accurate data base of 5200 HCN and HNC rotation-vibration energy levels, determined from existing laboratory data. 20 000 energy levels in the…”
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2
A H13CN/HN13C linelist, model atmospheres and synthetic spectra for carbon stars
Published in Monthly notices of the Royal Astronomical Society (11-10-2008)“…A linelist of vibration–rotation transitions for 13C substituted HCN is presented. The linelist is constructed using known experimental levels where available,…”
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3
UKRVO SPECTRAL PHOTOGRAPHIC ARCHIVE OF VARIABLE STARS
Published in Odessa astronomical publications (24-11-2020)“…The overview of the content of an Archive of the spectral photographic observational data stored at the MAO NAS of Ukraine in 1965–1985 is presented. Being the…”
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The cool giant HD 77361—a super Li-rich star
Published in Astronomy letters (01-12-2015)“…Super Li-rich stars form a very small and enigmatic group whose existence cannot be explained in terms of the standard stellar evolution theory. The goal of…”
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Analysis of the spectral energy distributions of four cool R CrB stars near the brightness maximum
Published in Astronomy reports (01-10-2013)“…The effective temperatures T eff and carbon and nitrogen abundances in the atmospheres of the cool R CrB stars ES Aql, SV Sge, Z UMi, and NSV 11154 have been…”
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Masses, Oxygen and Carbon abundances in CHEPS dwarf stars
Published 19-11-2018“…A&A 621, A112 (2019) Context. We report the results from the determination of stellar masses, carbon and oxygen abundances in the atmospheres of 107 stars from…”
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A detailed study of Lithium in 107 CHEPS dwarf stars
Published 18-10-2017“…A&A 611, A27 (2018) We report results from lithium abundance determinations using high resolution spectral analysis of the 107 metal-rich stars from the…”
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The Cool Giant HD 77361 - A Super Li-Rich Star
Published 05-02-2016“…Astronomy Letters, 2015, Vol. 41, No. 12, pp. 809-823 Super Li-rich stars form a very small and enigmatic group whose existence cannot be explained in terms of…”
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A H super(13)CN-HN super(13)C linelist, model atmospheres and synthetic spectra for carbon stars
Published in Monthly notices of the Royal Astronomical Society (11-10-2008)Get full text
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10
A H13CN/HN13C linelist, model atmospheres and synthetic spectra for carbon stars
Published 04-07-2008“…A line list of vibration-rotation transitions for 13C substituted HCN is presented. The line list is constructed using known experimental levels where…”
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11
A H13CN/HN13C linelist, model atmospheres and synthetic spectra for carbon stars
Published in Monthly notices of the Royal Astronomical Society (11-10-2008)Get full text
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12
A H 13 CN/HN 13 C linelist, model atmospheres and synthetic spectra for carbon stars
Published in Monthly notices of the Royal Astronomical Society (11-10-2008)Get full text
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13
Molecular line lists for modelling the opacity of cool stars
Published in Molecular physics (10-03-2007)“…The behaviour of cool stars is largely governed by molecular absorptions in their outer atmospheres. At the temperatures involved (1000 -- 4000 K), the number…”
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14
Improved HCN/HNC linelist, model atmospheres and synthetic spectra for WZ Cas
Published in Monthly notices of the Royal Astronomical Society (01-03-2006)Get full text
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15
Intraperitoneal drainage after pancreatic resection: a review of the evidence
Published in The Journal of surgical research (01-10-2013)“…Abstract Background Despite a growing body of literature supporting the limited use of prophylactic intra-abdominal drainage for many procedures, drain…”
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The absorption spectrum of V838 Mon in 2002 February–March — I. Atmospheric parameters and iron abundance
Published in Monthly notices of the Royal Astronomical Society (11-02-2005)“…We present a determination of the effective temperatures, iron abundances and microturbulent velocities for the pseudo-photosphere of V838 Mon on 2002 February…”
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The absorption spectrum of V838 Mon in 2002 February - March. I. Atmospheric parameters and iron abundance
Published 01-11-2004“…Mon.Not.Roy.Astron.Soc. 357 (2005) 38-44 We present a determination of the effective temperatures, iron abundances, and microturbulent velocities for the…”
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Improved HCN/HNC linelist, model atmospheres and synthetic spectra for WZ Cas
Published 14-12-2005“…Mon.Not.Roy.Astron.Soc.367:400-406,2006 We build an accurate database of 5200 HCN and HNC rotation-vibration energy levels, determined from existing laboratory…”
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19
The properties of V838 Mon in 2002 November
Published 08-09-2006“…We present the results of modelling the 0.45--1 micron spectral energy distribution of V838 Mon for 2002 November. Synthetic spectra were calculated using the…”
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