X-ray and ultraviolet data are presented with various optical data. Certain flare star and BY Draconis type variable star data are included. The results are discussed in terms of parameters of interest such as rotation and binary incidence. Deviations from correlations of properties that are found in the literature are noted. The fairly sizable number of red dwarfs that were observed inhance the value of the set of data. The coronae and the chromospheres of transition regions of the nearby stars are also considered
IUE data for X-ray binaries were collected and analyzed. Image processing was done for 144 IUE image...
We have suggested that cool magnetic white dwarfs may be sources of X-ray coronal emission and propo...
The details of a survey of the X-ray properties of ~65 dwarf novae are presented: four objects are d...
I analyse an x-ray selected sample of 128 late-type (F-M) stars. These stars were identified as opti...
The status of research undertaken with the IUE satellite for programs on strong binary X-ray stars a...
Ultraviolet studies of various astronomical entities are reported. Among the specific phenomena exam...
Just prior to the thesis research, an all-sky survey in hard x rays with the HEAO-1 satellite and fu...
We present the first study of nearby M dwarfs with the ROentgen Survey with an Imaging Telescope Arr...
Observational data for solar X-ray flares measured by Explorer 33 and Explorer 35 satellite
After presenting global properties of M dwarfs, the principal diagnostic of activity phenomena occur...
Progress in the EXOSAT data analysis program is reported. EXOSAT observations for four white dwarfs ...
The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and lum...
A search of all of the Einstein Observatory IPC and HRI fields for untargeted stars in the Woolley, ...
The purpose was to study various aspects of mass loss in stars of different types. The observational...
We present the results from a spectroscopic study of 1080 nearby active M dwarfs, selected by correl...
IUE data for X-ray binaries were collected and analyzed. Image processing was done for 144 IUE image...
We have suggested that cool magnetic white dwarfs may be sources of X-ray coronal emission and propo...
The details of a survey of the X-ray properties of ~65 dwarf novae are presented: four objects are d...
I analyse an x-ray selected sample of 128 late-type (F-M) stars. These stars were identified as opti...
The status of research undertaken with the IUE satellite for programs on strong binary X-ray stars a...
Ultraviolet studies of various astronomical entities are reported. Among the specific phenomena exam...
Just prior to the thesis research, an all-sky survey in hard x rays with the HEAO-1 satellite and fu...
We present the first study of nearby M dwarfs with the ROentgen Survey with an Imaging Telescope Arr...
Observational data for solar X-ray flares measured by Explorer 33 and Explorer 35 satellite
After presenting global properties of M dwarfs, the principal diagnostic of activity phenomena occur...
Progress in the EXOSAT data analysis program is reported. EXOSAT observations for four white dwarfs ...
The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and lum...
A search of all of the Einstein Observatory IPC and HRI fields for untargeted stars in the Woolley, ...
The purpose was to study various aspects of mass loss in stars of different types. The observational...
We present the results from a spectroscopic study of 1080 nearby active M dwarfs, selected by correl...
IUE data for X-ray binaries were collected and analyzed. Image processing was done for 144 IUE image...
We have suggested that cool magnetic white dwarfs may be sources of X-ray coronal emission and propo...
The details of a survey of the X-ray properties of ~65 dwarf novae are presented: four objects are d...