We report the detection of a photometric period of 3h09m23s from the optical counterpart of RX 11141.3- 6410. The amplitude of the optical modulation, 11m,...., 0.5 mag, and the period are consistent with the suggestion that this is an AM Herculis star. Quasi-periodic oscillations (QPOs) with time-scales in the range 20.0-42.1 min are also reported
T Pyx is one of four known recurrent novae suspected to be powered by thermonuclear runaways. If the...
Aims.Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 No. 1) performed during 12 nights...
We present extensive CCD photometry of the optical counterpart of X1735–444 which reveals the orbita...
CCD photometry of the classical nova RW UMi during 10 nights in 1995 through an R filter and 14 nigh...
curve with a prominent modulation on a period of 321.5 s. We present optical observations in which w...
We report detection of low-amplitude optical oscillations at periods of 312.77 s and 317.94 s of the...
We present the discovery of the photometric (orbital) period for V1974 Cygni (Nova Cygni 1992). The ...
We present high speed optical photometric observations made using the NTT and ULTRACAM of the optica...
We present high speed optical photometric observations made using the NTT and ULTRACAM of the optica...
Abstract. We report on the results of a spectroscopic and photometric study of a new cataclysmic var...
Aims. We wanted to determine the rotation parameters of GQ Lup A, thereby constraining the evolutio...
Aims. We attempt to establish the real nature of the orbital period variation and its relation to th...
A period study of the binary system TX Her based on the extensive series of minima times covering al...
A detailed orbital period investigation of the short-period ($P=0\fd 37$) W UMa type star, V417 Aql,...
We present a detailed time-resolved photometric study of the ultracompact X-ray binary candidate 4U ...
T Pyx is one of four known recurrent novae suspected to be powered by thermonuclear runaways. If the...
Aims.Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 No. 1) performed during 12 nights...
We present extensive CCD photometry of the optical counterpart of X1735–444 which reveals the orbita...
CCD photometry of the classical nova RW UMi during 10 nights in 1995 through an R filter and 14 nigh...
curve with a prominent modulation on a period of 321.5 s. We present optical observations in which w...
We report detection of low-amplitude optical oscillations at periods of 312.77 s and 317.94 s of the...
We present the discovery of the photometric (orbital) period for V1974 Cygni (Nova Cygni 1992). The ...
We present high speed optical photometric observations made using the NTT and ULTRACAM of the optica...
We present high speed optical photometric observations made using the NTT and ULTRACAM of the optica...
Abstract. We report on the results of a spectroscopic and photometric study of a new cataclysmic var...
Aims. We wanted to determine the rotation parameters of GQ Lup A, thereby constraining the evolutio...
Aims. We attempt to establish the real nature of the orbital period variation and its relation to th...
A period study of the binary system TX Her based on the extensive series of minima times covering al...
A detailed orbital period investigation of the short-period ($P=0\fd 37$) W UMa type star, V417 Aql,...
We present a detailed time-resolved photometric study of the ultracompact X-ray binary candidate 4U ...
T Pyx is one of four known recurrent novae suspected to be powered by thermonuclear runaways. If the...
Aims.Period analysis of CCD photometry of V1493 Aql (Nova Aql 1999 No. 1) performed during 12 nights...
We present extensive CCD photometry of the optical counterpart of X1735–444 which reveals the orbita...
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