Bartol Hot Star Preprints

NOTE: All files on this page are UNIX-compressed postscript files:

(i.e.,  file.ps.Z).

Papers available:

1. Hydrodynamical Simulations of Corotating Interaction Regions and Discrete Absorption Components in Rotating O-Star Winds, by Steven R. Cranmer and Stanley P. Owocki. Submitted to Ap. J. on July 31, 1995.
   • Main Text (89K)
   • Figure 1 (35K)
   • Figure 2 (23K)
   • Figure 3 (73K)
   • Figure 4 (94K)
   • Figure 5 (29K)
   • Figure 6 (46K)
   • Figure 7 (66K)
   • Figure 8 (37K)
   • Figure 9a (13K)
   • Figure 9b (13K)
   • Figure 9c (15K)
   • Figure 10 (11K)
   • Figure 11a (56K)
   • Figure 11b (63K)
   • Figure 12 (73K)
   • Figure 13a (19K)
   • Figure 13b (23K)
   • Figure 13c (23K)
   • Figure 14 (14K)

2. Periodic Variations in UV Spectral Lines of the B0.5~Ib Star HD~64760: Evidence for Corotating Wind Streams Rooted in Surface Variations, by Stanley P. Owocki, Steven R. Cranmer, and Alexander W. Fullerton. Submitted to Ap. J. Letters on June 26, 1995. Accepted on August 18, 1995.
   • Main Text (43K)
   • Figure 1 (49K)
   • Figure 2 (14K)
   • Figure 3 (29K)

3. The Importance of Radiative Braking for the Wind Interaction in the Close WR+O Binary V444 Cygni, by Stanley P. Owocki and Kenneth G. Gayley. Submitted to Ap. J. Letters on June 30, 1995.
   • Coming soon! For now, please email Ken Gayley for copies.

4. Evidence for Wind Attenuation and a Multi-Temperature Plasma in the Combined EUVE and ROSAT Observations of epsilon Canis Majoris (B2 II), by D. H. Cohen, R. G. Cooper, J. J. MacFarlane, S. P. Owocki, J. P. Cassinelli, & P. Wang. To appear in the Ap. J., March 20, 1996.
   • Postscript version of preprint directly available from Dave Cohen.

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