Doppler Tomography of Intermediate Polar Spin Cycles
Author(s) -
C. Hellier
Publication year - 1999
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/307345
Subject(s) - line (geometry) , intermediate polar , polar , tomography , white dwarf , physics , doppler effect , spin (aerodynamics) , phase (matter) , astrophysics , flux (metallurgy) , astronomy , stars , optics , materials science , geometry , mathematics , quantum mechanics , thermodynamics , metallurgy
I collect emission line profiles for seven intermediate polars,phase-resolved over the spin cycles. I then present the first systematicapplication of Doppler tomography to the spin cycles, with the aim ofinvestigating whether spin-cycle tomography is a useful diagnostic tool. Fourstars show line emission from material falling onto both magnetic poles of thewhite dwarf, but three others show line emission from only the upper pole.Tomography can map the extent and shape of the line-emitting accretioncurtains, but it can also give misleading results if the line flux changessignificantly over the spin cycle.
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