КНИГИ НА АНГЛИЙСКИЙ ЯЗЫКЕ, ИМЕЮЩЕЕ ОТНОШЕНИЕ К СЛОВУ «NOVALIKE»
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1
Close Binaries in the 21st Century: New Opportunities and ...
The. Structure. and. the. Partial. Opacity. of. the. Spiral. Shocks. on. the. Novalike.
Cataclysmic. Variables. Deductions from the Indication of Eclipses of Nova
V1493 Aql. DOI 10.1007/s10509-006-9140-x ORIGINAL ARTICLE Christos ...
Alvaro Giménez, Àlvaro Giménez, Edward Guinan, 2007
2
Cataclysmic Variable Stars - How and Why They Vary
5.16: The orbital periods of dwarf novae, Z Cam stars and novalike variables,
from a compilation by Hans Ritter and Uli Kolb.14 novae, and also found stars
which were similar to the remnants of past novae. They called these 'nova-like ...
3
Advances in Stellar Evolution
An. Analysis. of. Long-term. Light. Curves. of. Four. Novalike. Variables. By.
ZDRAVKA KRAICHEVA1f, VALLERY STANISHEV1, IGLIKA SPASSOVSKA2
AND VASIL POPOV1 1institute of Astronomy, Bulgarian Academy of Sciences, ...
Robert T. Rood, Alvio Renzini, 1997
4
Observing Variable Stars
The Roche-overflow gas from the secondary star forms an accretion disk around
the compact object. The chief source of the visual light of DNs is from the
accretion disks. The group of stars known as V Sagittae stars are classified as
novalike, ...
5
Accretion-powered Compact Binaries
The mass-transfer rates of quiescent novae and novalike systems are believed to
be more stable than dwarf novae. They may however show cyclical variations of
their quiescent luminosity on timescales of years (Bianchini 1989a). The disk ...
Christopher W. Mauche, 2003
6
Visit to Small Universe
Included are novae, dwarf novae, recurrent novae, novalike variables, symbiotic
stars, and polars. All show slight, rapid flickering, and some, of course, explode.
Two different energy sources are involved. First, gas dropping down toward the ...
7
Non-Solar X- and Gamma-Ray Astronomy
To my continuing program of photoelectric observations of novalike variables, I
have added certain optically identified X-ray sources because the two classes of
objects appear to be photometrically similar. The data for Cyg X-2 were obtained
...
Livio Gratton, International Astronomical Union, 1970
8
Binary Stars: Selected Topics on Observations and Physical ...
[2] applied this method to HST data of the eclipsing novalike variable, UX UMa.
Examples of the light curves and the final spectra they derived are plotted in Fig.
4.6. These spectra clearly show the increase of intensity as one moves from the ...
F. C. Lazaro, M.J. Arevalo, 2001
Q Novae, dwarf novae Object Kuwano, a novalike (symbiotic?! binary with a red
giant: photometry and polarimetry. — T. S. Belyakina, Yu. S. Efimov, E. P.
Pavlenko, and V. I. Shenavrin; 26 (1), 1-3. Object Kuwano, a novalike (symbiotic?
) binary ...
10
Light Curves of Variable Stars: A Pictorial Atlas
... SD semi-detached systems' Table 1.7 X-ray sources Variables GC VS XB X-ray
bursters XF fluctuating X-ray systems XI X-ray irregulars XJ X-ray binaries with
relativistic jets XND X-ray novalike with late-type component XNG X-ray novalike
...
C. Sterken, C. Jaschek, 2005
