Browsing by Author "Bennett, Philip Desmond, 1952-"

Browsing by Author "Bennett, Philip Desmond, 1952-"

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    An atlas of far-ultraviolet spectra of the Zeta Aurigae binary 31 Cygni with line identifications 
    Hagen Bauer, Wendy; Bennett, Philip Desmond, 1952- (IOP Publishing, 2014-04)
    The ζ Aurigae system 31 Cygni (K4 Ib + B4 V) was observed by the FUSE satellite during total eclipse and at three phases during chromospheric eclipse. We present the coadded, calibrated spectra and atlases with line ...

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    Epsilon Aurigae : deriving a Baade-Wesselink distance 
    Wilson, Christine K. (Halifax, N.S. : Saint Mary's University, 2013)
    Epsilon Aurigae is a third magnitude, long-period binary that eclipses every 27.1 years and has been continuously observed for more than 160 years. The observed spectrum is that of an apparently normal F supergiant. The ...

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    The long-term binary system VV Cep 
    Pollmann, E; Bennett, Philip Desmond, 1952-; Hopkins, J. L. (Konkoly Observatory, 2016-01-16)
    VV Cep is an eclipsing binary with a period of about 20.4 years that is comprised of an M2Iab primary star and an early B secondary star. A preliminary orbit was announced in 1933 by Harper & Christie (1936), and McLaughlin ...

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    Orbitally modulated photoexcited Si I emission in the eclipsing composite-spectrum binary [zeta] Aurigae 
    Harper, G. M.; Griffin, R. E. M.; Bennett, Philip Desmond, 1952-; O'Riain, N. (Oxford University Press, 2016-02-21)
    We examine the little-known phenomenon of orbitally modulated Si I emission at [lambda] 3905.523 [angstrom] and [lambda] 4102.936 [angstrom] in composite-spectrum binaries, with specific reference to [zeta] Aurigae (K4 Ib ...

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    Spectral and photometric analysis of the eclipsing binary [epsilon] Aurigae prior to and during the 2009–2011 eclipse 
    Chadima, P.; Harmanec, P.; Bennett, Philip Desmond, 1952-; Kloppenborg, B.; Stencel, R.; Yang, S.; Bozic, H.; Slechta, M.; Kotkova, L.; Wolf, M. (EDP Sciences, 2011-06)
    A series of 353 red electronic spectra (from three observatories, mostly from 6300 to 6700 A) obtained between 1994 and 2010, and of 171 UBV photometric observations (from two observatories) of the 2010 eclipse, were ...