[PDF] Top 20 Photometric Analysis of Eclipsing Binary Stars
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Photometric Analysis of Eclipsing Binary Stars
... of binary stars is vitally important in astronomy because it is only by carefully measuring the interactions between stars that we can accurately determine their absolute characteristics such as ... See full document
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The binary properties of the pulsating subdwarf B eclipsing binary PG 1336 018 (NY Virginis)
... current binary analysis codes, which also prevented us to pinpoint the effective temperature of the sec- ...the analysis methods available in the literature treat the atmosphere of such a close ... See full document
12
Eclipsing binaries observed with the WIRE satellite I, Discovery and photometric analysis of the new bright A0 IV eclipsing binary ψ Centauri
... As can be seen from Table 2, the fractional radii of the com- ponent stars of ψ Cen are known to impressive random errors of 0.10% (primary star) and 0.15% (secondary), and all of the light curve parameters are ... See full document
9
USING APASS STANDARDS TO TRANSFORM CCD OBSERVATIONS:
... of eclipsing binary stars as differ- ential magnitudes of the target star against a comparison star, the observations reported herein have been transformed to the standard (Vega) system using on-chip ... See full document
6
A Wind analysis of an evolved Giant FUSE and HST/STIS observations of an eclipsing Symbiotic Binary
... Symbiotic systems can be used as laboratories in which to perform detailed studies on giant winds in ways which would not be possible for isolated stars. Effects due to the presence of an ionising source close to ... See full document
9
A holistic study of the eclipsing binary EQ Tau
... calculated photometric elements resulting from their observations with published spectroscopic elements to yield the absolute parameters of the ...Many photometric studies were applied for the system light ... See full document
21
Photometric Study of Three Short Period Eclipsing Binaries from the ASAS Catalogue
... The photometric data for ASAS 105331 − ...the analysis of the ...over-contact binary star of the W Uma type comprising two main sequence ...The photometric mass ratio was determined to be ... See full document
8
A search for photometric variability towards M71 with the Near-Infrared Transiting ExoplanetS Telescope
... variable stars v38 and v30, one is the probable eclipsing binary v10 of PN00 (which is confirmed here) and the light curves of the remaining two objects are inconsistent with giant transiting ... See full document
16
A magnetic white dwarf in a detached eclipsing binary
... detached, eclipsing white dwarf plus M dwarf binary which shows a large infrared excess which has been interpreted in terms of a circumbinary dust ...near-infrared photometric and spectroscopic data ... See full document
12
A magnetic white dwarf in a detached eclipsing binary
... detached, eclipsing white dwarf plus M dwarf binary which shows a large infrared excess which has been interpreted in terms of a circumbi- nary dust ...near-infrared photometric and spectro- scopic ... See full document
15
Spectroscopic Analysis of Eclipsing Binary Stars
... the binary components, we adjusted a numerical eclipsing binary model to the observations; the mass-ratio of ER Vul and BX And were fixed at the values of ... See full document
8
The EBLM project : II A very hot, low mass M dwarf in an eccentric and long period, eclipsing binary system from the SuperWASP survey
... dex), eclipsing binary in an eccentric orbit ( ∼ ...d. Eclipsing M dwarfs that orbit solar-type stars (EBLMs), like J0113 + 31, have been identified from their light curves and follow-up ... See full document
13
HATS-31b through HATS-35b: five transiting hot Jupiters discovered by the HATSouth survey
... Our analysis of the combined photometric and spectroscopic data rules out the possibility that these transit detections are blended stellar eclipsing binary systems, and we conclude that these ... See full document
16
The Pan-Pacific planet search. V. Fundamental parameters for 164 evolved stars
... evolved stars, many of which represent the fi rst such ...complete analysis of the occurrence rate of planets in the PPPS sample is beyond the scope of this work, and indeed is premature as we are continuing ... See full document
15
PERIODIC HEMISSION IN THE ECLIPSING BINARY VV CEPHEI
... In structure, the Hα emission line appears doubled with two prominent peaks separated by self-absorption near line center (Fig. 2). Wright (1977) assumed that this profile was due to a single, intrinsic symmetric ... See full document
9
The Wolf-Rayet population of the nearby barred spiral galaxy NGC 5068 uncovered by the Very Large Telescope and Gemini
... An alternative scenario for the production of Type Ib/c ccSNe has been proposed by Podsialowski, Joss & Hsu (1992) in which intermediate-mass stars in binary systems lose their hydrogen and helium ... See full document
17
Synergies between exoplanet surveys and variable star research
... many stars as possible for at least a period of a few ...and analysis methods, leading to better than 1% per data point precision for thousands of ...the photometric satellites CoRoT and Kepler, the ... See full document
13
A New Detached M Dwarf Eclipsing Binary
... dwarf eclipsing binary ...nights. Analysis of the folded light curve indicates two very similar components orbiting each other with a period of ... See full document
5
Eclipsing Am binary systems in the SuperWASP survey
... of eclipsing Am stars found by WASP does ap- pear to be broadly consistent with the expected number of sys- ...the eclipsing fraction appears to be similar, suggesting a significant fraction of Am ... See full document
20
On the dynamical stability of the proposed planetary system orbiting NSVS 14256825
... B stars are highly uncertain (Hu et ...close binary progenitors of these post-common-envelope systems show that the initial mass distribution of primary stars that result in subdwarf B stars ... See full document
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