Broad-Band Variability in Accreting Compact Objects
Cataclysmic variable stars are in many ways similar to X-ray binaries. Both types of systems possess an accretion disk, which in most cases can reach the surface (or event horizon) of the central compact object. The main difference is that the embedded gravitational potential well in X-ray binaries...
Saved in:
| Main Author: | S. Scaringi |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Czech Technical University in Prague
2015-02-01
|
| Series: | Acta Polytechnica CTU Proceedings |
| Online Access: | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2850 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Broad angle broadband resolver for THz band
by: Yasith Amarasinghe, et al.
Published: (2025-07-01) -
Bolometric Corrections for FU Ori Object Accretion Disk Luminosities
by: Adolfo S. Carvalho, et al.
Published: (2024-01-01) -
Analysis of broad-band piezoelectric sandwich transducer with perforated structure
by: Chong-Mao LI, et al.
Published: (2015-07-01) -
Broad Observational Perspectives Achieved by the Accreting White Dwarf Sciences in the <i>XMM-Newton</i> and <i>Chandra</i> Eras
by: Şölen Balman, et al.
Published: (2025-03-01) -
Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity
by: Salvatore Orlando, et al.
Published: (2014-12-01)