Ograniczanie wyników
Preferencje help
Widoczny [Schowaj] Abstrakt
Liczba wyników

Znaleziono wyników: 2

Liczba wyników na stronie
first rewind previous Strona / 1 next fast forward last
Wyniki wyszukiwania
Wyszukiwano:
w słowach kluczowych:  stars: individual: Z Cha
help Sortuj według:

help Ogranicz wyniki do:
first rewind previous Strona / 1 next fast forward last
1
Content available remote Stream Overflow in Z Cha and OY Car during Quiescence
EN
Eclipses of the hot spot in Z Cha and OY Car observed by many authors during their quiescence are re-analyzed. Distances of the spot from the center of the disk rs are determined from phases of ingress and egress. In the case of several eclipses of Z Cha and nearly all eclipses of OY Car it is found that rs(egress)s(ingress). This is interpreted as being due to the effects of stream overflow and implies that those values of rs are not representative for the radius of the disk rd. The rs(ingress)-dt relations (where dt is the time since last outburst) are improved when points affected by the stream overflow are omitted.
EN
Observational data for five dwarf novae of the SU UMa type provide several strong arguments in favor of a significant enhancement in the mass transfer rate during their outbursts and superoutbursts. The mass transfer rates during normal outbursts are estimated from the amount of accreted mass assuming the theoretical mass transfer rate at quiescence, based on models involving gravitational waves. The resulting rates Menh≈0.6-1.8×1017 g/s imply enhancement by a factor of 15-46, which is consistent with observational evidence for VW Hyi and with theoretical predictions. The mass transfer rates during superoutbursts are enhanced to Menh≈3-6×1017 g/s. The corresponding enhancement ratios range from ≈20-60 (when the mass transfer rates at quiescence are obtained under assumption of no enhancement during normal outbursts) up to ≈100 (resulting from the assumption of the theoretical mass transfer rate during quiescence).
first rewind previous Strona / 1 next fast forward last
JavaScript jest wyłączony w Twojej przeglądarce internetowej. Włącz go, a następnie odśwież stronę, aby móc w pełni z niej korzystać.