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Publication
Featured researches published by Gary E. Walker.
The Astrophysical Journal | 1999
Paula Szkody; Albert P. Linnell; Kent Honeycutt; J. W. Robertson; Andrew D. Silber; Donald Wayne Hoard; Lora Pastwick; Vandana Desai; Ivan Hubeny; John K. Cannizzo; William Liller; Ronald E. Zissell; Gary E. Walker
A complete 45 day supercycle of the cataclysmic variable V1159 Ori comprising a superoutburst and eight normal outbursts was observed. Coverage included ground-based optical observations as well as observations with RXTE for 38 days, ROSAT for 34 days, IUE for 27 days, and Extreme Ultraviolet Explorer (EUVE) for 10 days. The resulting light curves reveal that the optical and UV light variations are inversely correlated with the RXTE and ROSAT fluxes, with the largest change in intensity occurring in the ROSAT bandpass. There is no evidence for a strong EUV/soft X-ray component during outburst. An outflowing wind is evident from the C IV line profile during each brief outburst as well as the superoutburst. The transitions from outburst states of the disk to quiescent states take place on timescales of hours. Accretion disk models can fit the UV line and continuum energy distributions near outburst only if the disk radial temperature profile is modified from the standard case to produce a hotter distribution in the outer annuli. The high mass transfer rate, the hot disk distribution, and the similarity of outbursts and superoutbursts argue for outside-in outbursts in this system.
Proceedings of the International Astronomical Union | 2010
Vladimir S. Strelnitski; Kamber Schwarz; John H. Bieging; Josh T. Fuchs; Gary E. Walker
MWC349A, which had remained an ordinary member of the MWC catalog for a few decades, is now known as: (1) the brightest stellar source of radio continuum; (2) the only known high-gain natural maser in hydrogen recombination lines; and (3) the only strictly proven natural high-gain laser (in IR hydrogen recombination lines). These phenomena seem to occur in the circumstellar disk seen almost edge-on. They help us understand the structure and kinematics of the disk. The evolutionary status of MWC 349A is still debated: a young HAeBe star with a pre-planetary disk or an old B[e] star or even a protoplanetary nebula? We discuss new observational data obtained at the Maria Mitchell Observatory and elsewhere which may cast light on this issue.
The Astrophysical Journal | 2013
Svetlana G. Jorstad; Alan P. Marscher; Paul S. Smith; Valeri M. Larionov; I. Agudo; M. A. Gurwell; Ann E. Wehrle; A. Lähteenmäki; Maria G. Nikolashvili; Gary D. Schmidt; A. A. Arkharov; D. Blinov; Kelly Blumenthal; C. Casadio; R. A. Chigladze; N. V. Efimova; Joseph R. Eggen; José L. Gómez; Dirk Grupe; V. A. Hagen-Thorn; M. Joshi; G. N. Kimeridze; T. S. Konstantinova; E. N. Kopatskaya; Omar M. Kurtanidze; S. O. Kurtanidze; Elena G. Larionova; L. V. Larionova; L. A. Sigua; Nicholas R. MacDonald
The Astronomical Journal | 1996
Steve B. Howell; James Deyoung; Janet Akyuz Mattei; Grant Foster; Paula Szkody; John K. Cannizzo; Gary E. Walker; Erik Fierce
The Astrophysical Journal | 2013
Vladimir S. Strelnitski; John H. Bieging; Joseph L. Hora; H. A. Smith; Peter Armstrong; Krister Lagergren; Gary E. Walker
The Astronomical Journal | 2011
Megan E. Bedell; Alexa Villaume; Lauren M. Weiss; Vladimir S. Strelnitski; Gary E. Walker; Jedediyah Williams; Arne A. Henden; Tom Krajci
Bulletin of the American Physical Society | 2018
Eydon Thomashow; Regina A. Jorgenson; Vladimir S. Strelnitski; Gary E. Walker
Archive | 2011
Megan E. Bedell; Alexa Villaume; Vladimir S. Strelnitski; Gary E. Walker
Archive | 2011
Kamber Schwarz; Vladimir S. Strelnitski; Gary E. Walker
Archive | 2011
Stephanie Sallum; Svetlana G. Jorstad; Alan P. Marscher; Gary E. Walker; Vladimir S. Strelnitski; Valeri M. Larionov