Received: 2015-7-27
Accepted: 2015-8-31
Published Online: 2017-2-18
Published in Print: 2015-9-1
© 2015 M. R. Sanad, published by De Gruyter Open
Artikel in diesem Heft
- Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
- Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3
- Optics for Nano-Satellite X-Ray Monitor
- Observational Data and Orbits of the Asteroids Discovered at the Baldone Observatory in 2008–2013
- On the Pseudo Phase-space Density of Dark Matter Haloes and the Universality of Density Profiles
- Baryon Physics and the Missing Satellites Problem
- A Young Star Cluster in the Leo a Galaxy
- Supershells in the M33 Galaxy
- Structural Parameters of Star Clusters: Signal to Noise Effects
- Artificial Star Test for Crowded Field CCD Photometry
- Ultraviolet and Infrared Correlation Studies in Orion
- Ultraviolet Spectroscopic Investigation of HU Aqr and AN UMa with the Data from HST and IUE
Schlagwörter für diesen Artikel
accretion;
stars: individual (HU Aqr, AN UMa);
cataclysmic variables;
ultraviolet: stars
Creative Commons
BY-NC-ND 3.0
Artikel in diesem Heft
- Stochastic 2-D Galaxy disk Evolution Models. Resolved Stellar Populations in the Galaxy M33
- Structural and Morphological Properties of Ultraluminous Infrared Galaxies at 1 < z < 3
- Optics for Nano-Satellite X-Ray Monitor
- Observational Data and Orbits of the Asteroids Discovered at the Baldone Observatory in 2008–2013
- On the Pseudo Phase-space Density of Dark Matter Haloes and the Universality of Density Profiles
- Baryon Physics and the Missing Satellites Problem
- A Young Star Cluster in the Leo a Galaxy
- Supershells in the M33 Galaxy
- Structural Parameters of Star Clusters: Signal to Noise Effects
- Artificial Star Test for Crowded Field CCD Photometry
- Ultraviolet and Infrared Correlation Studies in Orion
- Ultraviolet Spectroscopic Investigation of HU Aqr and AN UMa with the Data from HST and IUE