Just prior to the thesis research, an all-sky survey in hard x rays with the HEAO-1 satellite and further observations in the optical resulted in a catalog of about 700 x-ray sources with known optical counterparts. This sample includes 43 cataclysmic variables, which are binaries consisting of a detached white-dwarf and a Roche lobe filling companion star. This thesis consists of studies of the x-ray selected sample of catalcysmic variables
The x-ray emissions of AM Herculis-type object H0538+608 were observed using the ROSAT satellite. Ev...
The purpose of this study is to identify Cataclysmic Variables (CVs) using spectroscopic and photome...
We present photometry and spectroscopy of 11 and 35 potential cataclysmic variables, respectively, f...
The high energy emissions from cataclysmic variables (interacting binary systems containing an accre...
We report on ground-based optical observations of 10 cataclysmic binaries that were discovered throu...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
In cataclysmic variables (CVs), accretion onto white dwarfs produces high temperature, high density ...
CVs are interacting binaries accreting through Roche lobe overflow. The main motivation of this thes...
This paper completes the series of cataclysmic variables (CVs) identified from the Sloan Digital Sky...
The past and current projects of the Sloan Digital Sky Survey are reviewed in the context of applica...
From a set of 13 cataclysmic binaries that were discovered in the Swift Burst Alert Telescope (BAT) ...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
We measure the spatial distribution and hard X-ray luminosity function of cataclysmic variables (CVs...
The commissioning year of the Sloan Digital Sky Survey has demonstrated that many cataclysmic variab...
This paper identifies the cataclysmic variables that appear in spectra obtained in 2004 as part of t...
The x-ray emissions of AM Herculis-type object H0538+608 were observed using the ROSAT satellite. Ev...
The purpose of this study is to identify Cataclysmic Variables (CVs) using spectroscopic and photome...
We present photometry and spectroscopy of 11 and 35 potential cataclysmic variables, respectively, f...
The high energy emissions from cataclysmic variables (interacting binary systems containing an accre...
We report on ground-based optical observations of 10 cataclysmic binaries that were discovered throu...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
In cataclysmic variables (CVs), accretion onto white dwarfs produces high temperature, high density ...
CVs are interacting binaries accreting through Roche lobe overflow. The main motivation of this thes...
This paper completes the series of cataclysmic variables (CVs) identified from the Sloan Digital Sky...
The past and current projects of the Sloan Digital Sky Survey are reviewed in the context of applica...
From a set of 13 cataclysmic binaries that were discovered in the Swift Burst Alert Telescope (BAT) ...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
We measure the spatial distribution and hard X-ray luminosity function of cataclysmic variables (CVs...
The commissioning year of the Sloan Digital Sky Survey has demonstrated that many cataclysmic variab...
This paper identifies the cataclysmic variables that appear in spectra obtained in 2004 as part of t...
The x-ray emissions of AM Herculis-type object H0538+608 were observed using the ROSAT satellite. Ev...
The purpose of this study is to identify Cataclysmic Variables (CVs) using spectroscopic and photome...
We present photometry and spectroscopy of 11 and 35 potential cataclysmic variables, respectively, f...