Authors:
QUIRRENBACH A
BJORKMAN KS
BJORKMAN JE
HUMMEL CA
BUSCHER DF
ARMSTRONG JT
MOZURKEWICH D
ELIAS NM
BABLER BL
Citation: A. Quirrenbach et al., CONSTRAINTS ON THE GEOMETRY OF CIRCUMSTELLAR ENVELOPES - OPTICAL INTERFEROMETRIC AND SPECTROPOLARIMETRIC OBSERVATIONS OF 7 BE STARS, The Astrophysical journal, 479(1), 1997, pp. 477-496
Citation: K. Wood et al., DERIVING THE GEOMETRY OF BE STAR CIRCUMSTELLAR ENVELOPES FROM CONTINUUM SPECTROPOLARIMETRY .1. THE CASE OF XI-TAURI, The Astrophysical journal, 477(2), 1997, pp. 926-939
Citation: K. Wood et al., THE EFFECT OF MULTIPLE-SCATTERING ON THE POLARIZATION FROM AXISYMMETRICAL CIRCUMSTELLAR ENVELOPES .1. PURE THOMSON SCATTERING ENVELOPES, The Astrophysical journal, 461(2), 1996, pp. 828-846
Citation: K. Wood et al., THE EFFECT OF MULTIPLE-SCATTERING ON THE POLARIZATION FROM AXISYMMETRICAL CIRCUMSTELLAR ENVELOPES .2. THOMSON SCATTERING IN THE PRESENCE OFABSORPTIVE OPACITY SOURCES, The Astrophysical journal, 461(2), 1996, pp. 847-857
Citation: Je. Bjorkman, THE SOLUTION TOPOLOGY OF RADIATION-DRIVEN WINDS .1. THE X-TYPE NATUREOF THE CAK CRITICAL-POINT, The Astrophysical journal, 453(1), 1995, pp. 369-379
Citation: K. Wood et Je. Bjorkman, EFFECTS OF PRESCATTERING ATTENUATION ON SPECTROPOLARIMETRIC LINE-PROFILES, The Astrophysical journal, 443(1), 1995, pp. 348-362
Citation: Je. Bjorkman et Ks. Bjorkman, THE EFFECTS OF GRAVITY DARKENING ON THE ULTRAVIOLET CONTINUUM POLARIZATION PRODUCED BY CIRCUMSTELLAR DISKS, The Astrophysical journal, 436(2), 1994, pp. 818-830
Authors:
BJORKMAN JE
IGNACE R
TRIPP TM
CASSINELLI JP
Citation: Je. Bjorkman et al., EVIDENCE FOR A DISK IN THE WIND OF HD-93521 - UV LINE-PROFILES FROM AN AXISYMMETRICAL MODEL, The Astrophysical journal, 435(1), 1994, pp. 416-434
Authors:
BJORKMAN JE
IGNACE R
TRIPP TM
CASSINELLI JP
Citation: Je. Bjorkman et al., EVIDENCE FOR A DISK IN THE WIND OF HD-93521 - UV LINE-PROFILES FROM AN AXISYMMETRICAL MODEL, The Astrophysical journal, 435(1), 1994, pp. 416-434
Citation: Je. Bjorkman et Jp. Cassinelli, EQUATORIAL DISK FORMATION AROUND ROTATING STARS DUE TO RAM PRESSURE CONFINEMENT BY THE STELLAR WIND, The Astrophysical journal, 409(1), 1993, pp. 429-449