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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Hellier 1999
- Bibinfo (this paper at ADS)
- Hellier, C. 1999, ApJ 519, 324-331.
- Type
- Observational: Spin tomography of IPs.
- Object(s)
- FO Aqr,
V1025 Cen,
BG CMi,
PQ Gem,
EX Hya,
V2400 Oph, and
AO Psc.
- Results
- Spin tomography (of H-beta and/or HeII 4696) shows upper curtain
emissions only in AO Psc, FO Aqr, and BG CMi; the emission is azimuthally
extended, and predominantly at low velocities (i.e., the outer parts).
PQ Gem has emission lines from both curtains, with an unusual phasing.
Two curtains are probably seen in V2400 Oph. In EX Hya, and also probably
in V1025 Cen, the emission lines are formed closer in, in both curtains.
General caution: tomography can't handle line intensity changes
(i.e., optically thick lines).
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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