Spectroscopy and orbital periods of the old novae V533 Herculis, V446 Herculis and X Serpentis
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[1] J. Thorstensen,et al. Spectroscopy of the Cataclysmic Binaries CY Lyrae, TW Trianguli, and VW Vulpeculae , 1998 .
[2] C. Hellier. V1315 Aquilae and the Nature of SW Sextantis Stars , 1996 .
[3] J. B. Hutchings. THE CATACLYSMIC VARIABLE BINARY V533 HERCULIS (NOVA 1963). , 1987 .
[4] R. P. Kraft. Binary Stars among Cataclysmic Variables. III. Ten Old Novae. , 1964 .
[5] Brian Warner,et al. Absolute magnitudes of cataclysmic variables , 1987 .
[6] G. Williams. Spectroscopy of cataclysmic variables. I. Observations. , 1983 .
[7] J. Patterson. Rapid oscillations in cataclysmic variables. II. The 63 second oscillation of V533 Herculis. , 1979 .
[8] J. Thorstensen,et al. PG0027+260 : an example of a class of cataclysmic binaries with mysterious, but consistent, behavior , 1991 .
[9] A. Evans,et al. Cataclysmic Variables and Related Objects , 1996 .
[10] E. Herbst,et al. Ion-molecule calculation of the abundance ratio of CCD to CCH in dense interstellar clouds. , 1987, The Astrophysical journal.
[11] K. Sekiguchi. Identification of V1017 Sgr as a cataclysmic variable binary system with unusually long period , 1992, Nature.
[12] Joseph Patterson,et al. THE DQ HERCULIS STARS , 1994 .
[13] J. Patterson,et al. The evolution of cataclysmic and low-mass X-ray binaries. , 1984 .
[14] J. Thorstensen,et al. Orbital studies of cataclysmic binaries. I - AB Draconis and WW Ceti , 1985 .
[15] J. Thorstensen,et al. ORBITAL PERIODS FOR SEVEN DWARF NOVAE OF THE SU URSAE MAJORIS SUBCLASS FROM RADIAL VELOCITIES AT MINIMUM LIGHT , 1996 .
[16] J. Thorstensen,et al. LS Pegasi: A Low‐Inclination SW Sextantis–Type Cataclysmic Binary with High‐Velocity Balmer Emission‐Line Wings , 1998, astro-ph/9811339.
[17] E. L. Robinson,et al. The pulse-timing and emission-line orbits of the white dwarf in the cataclysmic variable AE Aquarii , 1991 .
[18] B. Lites,et al. Sunspot Umbral Oscillations in the Photosphere, Chromosphere, and Transition Region , 1986 .
[19] A reference catalogue and atlas of galactic novae , 1987 .
[20] K. Mukai,et al. The optical spectra of old novae , 1996 .
[21] J. Cannizzo. The accretion disk limit cycle model : toward an understanding of the long-term behavior of SS Cygni , 1993 .
[22] D. Schneider,et al. The magnetic maw of 2A 0311-22.7. , 1980 .
[23] T. Marsh,et al. V795 Her: an SW Sex star in the period gap? , 1996 .
[24] J. Thorstensen,et al. ORBITAL PERIODS OF THE DWARF NOVAE AR AND, AM CAS, AND PY PER , 1996 .
[25] A. Shafter. The Role of the Dwarf Nova Period Distribution in Understanding the Evolution of Cataclysmic Variables , 1992 .
[26] U. Kolb,et al. Catalogue of Cataclysmic Binaries, Low-Mass X-Ray Binaries and Related Objects , 1984 .
[27] A. Henden,et al. V446 Herculis (Nova Her 1960) Is an Optical Triple: Implications for the Resumption of Dwarf Nova Outbursts following the Nova , 1998 .
[28] J. Thorstensen,et al. Pulsations and Accretion Geometry in YY Draconis: A Study Based on Hubble Space Telescope Observations , 1997 .
[29] G. Turner,et al. Periodic Outbursts in the Old Nova V446 Herculis , 1995 .
[30] G. Vaucouleurs. The extragalactic distance scale. I. A review of distance indicators: zero points and errors of primary indicators. , 1978 .