AAS 202nd Meeting, May 2003
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All findings are embargoed until the time of presentation at the
meeting.
Session 30 Novae, Supernovae and Remnants
Poster, Tuesday, May 27, 2003,
10:00am-6:30pm, West Exhbit Hall
- 30.01 Q Cyg: outflow from a long period old nova
- S. Kafka (Indiana Univ.), C. Tappert (Universidad de Concepcion), R.K. Honeycutt (Indiana Univ.), A. Bianchini (Universita di Padova)
- 30.02 Measurement of Reactions on 30P for Nova Nucleosynthesis
- Z. Ma (U. Tennessee), M. W. Guidry (U. Tennessee & ORNL Physics Division*), W. R. Hix (U. Tennessee), M. S. Smith (ORNL Physics Division* & RIBENS Collaboration)
- 30.03 The 14O(alpha, 2p)16O Rate and its Implications for Novae and X-Ray Bursts
- L. Dessieux (Dept. Physics and Astronomy, U. Tennessee), M. S. Smith (ORNL Physics Division*), W. R. Hix (Dept. Physics and Astronomy, U. Tennessee), M. W. Guidry (Dept. Physics and Astronomy, U. Tennessee; ORNL Physics Division*)
- 30.04 Optical spectroscopy of high-redshift supernovae
- E. A. Smith (Vanderbilt University)
- 30.05 Analysis of the Nature and Growth Rates of Fluid Instabilities in Core Collapse Supernovae
- E. A. Raley, S. W. Bruenn (Florida Atlantic University)
- 30.06 The HeI Isoelectronic Sequence in Cloudy: Comparison with Observations
- R. L. Porter, G. J. Ferland (University of Kentucky, Physics & Astronomy Dept.)
- 30.07 Large HI Structures Adjacent to the Central and Southern Regions of the Cygnus Loop
- D.A. Leahy (University of Calgary)
- 30.08 The Shock Structure of Supernova Remnant IC443
- M. R. Haas (NASA-Ames), S. J. U. Higdon (Cornell), M. G. Burton (Univ. New South Wales), D. J. Hollenbach (NASA-Ames)
- 30.09 M1-92 and the Symbiotic Star MWC~560: Two Evolutionary Phases of the same Type of Object?
- S. Torres-Peimbert (IA-UNAM), A. Arrieta (STScI), L. Georgiev (IA-UNAM)
- 30.10 Non-Thermal X-ray Emission from the Galactic Supernova Remnants G156.2+5.7 and G266.2-1.2
- T.G. Pannuti, G.E. Allen (MIT)
- 30.11 A Very Young, Fast, Bipolar Outflow at the center of the Red Rectangle
- R. Sahai (Jet Proplusion Laboratory/ Caltech), C. Sanchez Contreras (Caltech)
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