UB Paderborn / Katalog / Suche / in CDI

1 – 25 von 44

Sortiert nach

Parameters of the X-ray binary system Scorpius X-1

Monthly notices of the Royal Astronomical Society, 2021-11, Vol.508 (1), p.1389-1403

2021

Link zum Volltext

Verfügbarkeit prüfen

Optical, J and K light curves of XTE J1118+480 = KV UMa: the mass of the black hole and the spectrum of the non-stellar component

Monthly notices of the Royal Astronomical Society, 2019-12, Vol.490 (3), p.3287-3308

2019

Link zum Volltext

Verfügbarkeit prüfen

I -band photometry of the quiescent black hole X-ray nova GROJ0422 + 32 = V518 Per: modelling of the orbital light curve and estimation of the black hole mass

Monthly notices of the Royal Astronomical Society, 2024-06, Vol.531 (4), p.4917-4928

2024

Link zum Volltext

Verfügbarkeit prüfen

Population synthesis of AX J1745.6−2901 X-ray nova-type binaries with rapidly decreasing orbital periods

Monthly notices of the Royal Astronomical Society, 2022-07, Vol.514 (4), p.5375-5384

2022

Link zum Volltext

Verfügbarkeit prüfen

Accretion disc in the massive V448 Cygni system

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.396 (3), p.1553-1558

2009

Link zum Volltext

Verfügbarkeit prüfen

Synthetic light curves of close binaries in a cool-disk model. The “hot line” and “hot spot” as visual indicators of interaction between the flow and disk

Astronomy reports, 2011-05, Vol.55 (5), p.425-436

Khruzina, T. S.

2011

Link zum Volltext

Verfügbarkeit prüfen

Study of the Rapid Variability of a Dwarf Nova SS Cyg at Different Brightness Levels

Astronomy reports, 2024-02, Vol.68 (2), p.129-160

2024

Link zum Volltext

Verfügbarkeit prüfen

Optical and J, K -photometry of the quiescent black hole X-ray nova A0620−00 in the passive and active states

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.483 (1), p.1067-1079

2019

Link zum Volltext

Verfügbarkeit prüfen

Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star

Astronomy reports, 2022, Vol.66 (4), p.348-358

2022

Link zum Volltext

Verfügbarkeit prüfen

Parameter Determination for the Eclipsing Long-Period Dwarf Nova EX Dra from Photometric Observations during Different Activity States of the System

Astronomy reports, 2019-07, Vol.63 (7), p.571-594

2019

Link zum Volltext

Verfügbarkeit prüfen

Analysis of Photometric Observations of the New Cataclysmic Variable ASASSN-13cx

Astronomy reports, 2018, Vol.62 (1), p.31-49

2018

Link zum Volltext

Verfügbarkeit prüfen

Photometric behavior of the cataclysmic variable SDSS J150240.98+333423.9/NZ Boo in quiescence

Astronomy reports, 2015-05, Vol.59 (5), p.366-384

2015

Link zum Volltext

Verfügbarkeit prüfen

Light-curve syntheses for close binary systems: Modeling spiral waves in an elliptical disk around a white dwarf

Astronomy reports, 2005-10, Vol.49 (10), p.783-800

Khruzina, T S

2005

Link zum Volltext

Verfügbarkeit prüfen

A photometric study of the eclipsing dwarf nova GY Cnc in quiescence and during an outburst

Astronomy reports, 2016-11, Vol.60 (11), p.971-995

2016

Link zum Volltext

Verfügbarkeit prüfen

Structure of the accretion disk in the cataclysmic variable UX uma in the transition to its quiescent state

Astronomy reports, 2007-04, Vol.51 (4), p.318-338

2007

Link zum Volltext

Verfügbarkeit prüfen

Changes in the parameters of the accretion disk around the dwarf nova SDSS J090350.73+330036.1 during an outburst

Astronomy reports, 2012-11, Vol.56 (11), p.819-842

2012

Link zum Volltext

Verfügbarkeit prüfen

The dwarf nova V1239 herculis in quiescence

Astronomy reports, 2015-04, Vol.59 (4), p.288-312

2015

Link zum Volltext

Verfügbarkeit prüfen

Light-curve synthesis for close binaries: An extended shock as an analog of a hot spot in cataclysmic variables

Astronomy reports, 2001-04, Vol.45 (4), p.255-268

Khruzina, T S

2001

Link zum Volltext

Verfügbarkeit prüfen

Interpretation of the light curves of quiescent X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system

Astronomy reports, 2005-02, Vol.49 (2), p.79-88

2005

Link zum Volltext

Verfügbarkeit prüfen

Light-curve synthesis for close binaries: Elliptical disk around a white dwarf

Astronomy reports, 2000-07, Vol.44 (7), p.446-459

Khruzina, T S

2000

Link zum Volltext

Verfügbarkeit prüfen

Accretion disk of the cataclysmic variable IY UMa in quiescence and its active state

Astronomy reports, 2008-10, Vol.52 (10), p.815-834

2008

Link zum Volltext

Verfügbarkeit prüfen

Interpretation of light curves of the cataclysmic variable OY Car in a model with shockless interaction between a gaseous stream and the disk

Astronomy reports, 2003-03, Vol.47 (3), p.214-231

2003

Link zum Volltext

Verfügbarkeit prüfen

Interpretation of orbital light curves of U Geminorum

Astronomy reports, 2003-10, Vol.47 (10), p.848-864

2003

Link zum Volltext

Verfügbarkeit prüfen

Synthetic Doppler tomograms of gas flows in the binary system IP Peg

Astronomy reports, 2001-11, Vol.45 (11), p.872-881

2001

Link zum Volltext

Verfügbarkeit prüfen

Light curve interpretation for “Quiescent” X-ray novae in a model with noncollisional interaction between the flow and disk. The system GU Mus = GRS 1124-68

Astronomy reports, 2003-08, Vol.47 (8), p.621-636

2003

Link zum Volltext

Verfügbarkeit prüfen

1 – 25 von 44

Suche als RSS-Feed

Suchergebnisse filtern

Filter anzeigen

Nur zeigen

Geprüft (Peer-Review)
(40)
Mit Volltextzugriff
(44)

Publikationsform

Artikel
(44)

Sprache

Erscheinungsjahr

n.n

Thema

15 weitere anzeigen...

Weniger anzeigen...

Neu hinzugefügt

... seit 30 Tagen
(2)

Menü

Weitere Dienste

Einstellungen

Parameters of the X-ray binary system Scorpius X-1

Optical, J and K light curves of XTE J1118+480 = KV UMa: the mass of the black hole and the spectrum of the non-stellar component

I -band photometry of the quiescent black hole X-ray nova GROJ0422 + 32 = V518 Per: modelling of the orbital light curve and estimation of the black hole mass

Population synthesis of AX J1745.6−2901 X-ray nova-type binaries with rapidly decreasing orbital periods

Accretion disc in the massive V448 Cygni system

Synthetic light curves of close binaries in a cool-disk model. The “hot line” and “hot spot” as visual indicators of interaction between the flow and disk

Study of the Rapid Variability of a Dwarf Nova SS Cyg at Different Brightness Levels

Optical and J, K -photometry of the quiescent black hole X-ray nova A0620−00 in the passive and active states

Parameters of X-Ray Binary Sco X-1 in the Model of Partial Filling of Roche Lobe by Optical Star

Parameter Determination for the Eclipsing Long-Period Dwarf Nova EX Dra from Photometric Observations during Different Activity States of the System

Analysis of Photometric Observations of the New Cataclysmic Variable ASASSN-13cx

Photometric behavior of the cataclysmic variable SDSS J150240.98+333423.9/NZ Boo in quiescence

Light-curve syntheses for close binary systems: Modeling spiral waves in an elliptical disk around a white dwarf

A photometric study of the eclipsing dwarf nova GY Cnc in quiescence and during an outburst

Structure of the accretion disk in the cataclysmic variable UX uma in the transition to its quiescent state

Changes in the parameters of the accretion disk around the dwarf nova SDSS J090350.73+330036.1 during an outburst

The dwarf nova V1239 herculis in quiescence

Light-curve synthesis for close binaries: An extended shock as an analog of a hot spot in cataclysmic variables

Interpretation of the light curves of quiescent X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system

Light-curve synthesis for close binaries: Elliptical disk around a white dwarf

Accretion disk of the cataclysmic variable IY UMa in quiescence and its active state

Interpretation of light curves of the cataclysmic variable OY Car in a model with shockless interaction between a gaseous stream and the disk

Interpretation of orbital light curves of U Geminorum

Synthetic Doppler tomograms of gas flows in the binary system IP Peg

Light curve interpretation for “Quiescent” X-ray novae in a model with noncollisional interaction between the flow and disk. The system GU Mus = GRS 1124-68

Suchergebnisse filtern