X-Ray Binary
CHF 53.20
Auf Lager
SKU
BRQU113MBOB
1 Verfügbar 
Kostenloser Versand
Geliefert zwischen Mi., 08.10.2025 und Do., 09.10.2025
Details
High Quality Content by WIKIPEDIA articles! X-ray binaries are a class of binary stars that are luminous in X-rays. The X-rays are produced by matter falling from one component, called the donor (usually a relatively normal star) to the other component, called the accretor, which is compact: a white dwarf, neutron star, or black hole. The infalling matter releases gravitational potential energy, up to several tenths of its rest mass, as X-rays. An estimated 1041 positrons escape per second from a typical hard LMXB. X-ray binaries are further subdivided into several (sometimes overlapping) subclasses, that perhaps reflect the underlying physics better. Note that the classification by mass (high, intermediate, low) refers to the optically visible donor, not to the compact X-ray emitting accretor.
30 Tage Rückgaberecht
GarantieWeitere Informationen
- Allgemeine Informationen
- GTIN 09786131411267
- Editor Lambert M. Surhone, Mariam T. Tennoe, Susan F. Henssonow
- Genre Physik & Astronomie
- EAN 9786131411267
- Titel X-Ray Binary
- Herausgeber Betascript Publishing
- Anzahl Seiten 124
Bewertungen
Schreiben Sie eine Bewertung
