IPs
AE Aqr
FO Aqr
XY Ari
V405 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2306 Cyg
YY Dra
PQ Gem
DQ Her
EX Hya
NY Lup
V2400 Oph
GK Per
AO Psc
WX Pyx
V1223 Sgr
V1062 Tau
EI UMa
IGR 00234
IGR 15094
IGR 17303
Swift J0732
RX J0704
RX J1803
RX J2133
XSS 00564
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Eracleous & Horne 1996
- Bibinfo (this paper at ADS)
- Eracleous, M., Horne, K. 1996, ApJ 471, 427-446.
- Type
- Observational: Time-resolved UV spectroscopy.
- Object(s)
- AE Aqr.
- Results
- Studies of UV flares. Continuum and lines vary together. UV lines
lag the companion by about 1/3 of a cycle. Flares can be interpreted
as blobs encountering the propeller; work spent expelling the blobs
can explain the spin-down.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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