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[PDF] Top 20 Spectroscopic Analysis of Eclipsing Binary Stars

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Spectroscopic Analysis of Eclipsing Binary Stars

Spectroscopic Analysis of Eclipsing Binary Stars

... velocity analysis of the eclipsing binaries ER Vul and BX And are presented and ...The analysis of spectroscopic data of both eclipsing binaries using PHOEBE, BM3 and SBS models has ... See full document

8

A magnetic white dwarf in a detached eclipsing binary

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 ...Our spectroscopic observations reveal Zeeman ... See full document

15

A New Detached M Dwarf Eclipsing Binary

A New Detached M Dwarf Eclipsing Binary

... obtained spectroscopic observations of TrES-Her0-07621 using the High Resolution Spectrograph (HRS; Tull 1998) on the Hobby-Eberly Telescope ...The analysis was carried out with standard IRAF (Tody 1993) ... See full document

5

PERIODIC HEMISSION IN THE ECLIPSING BINARY VV CEPHEI

PERIODIC HEMISSION IN THE ECLIPSING BINARY VV CEPHEI

... long-term spectroscopic monitoring program of the Hα emission line of VV ...Cephei. Spectroscopic observations have been obtained on a regular basis of the red spectral region around Hα, on a regular basis ... See full document

9

The binary properties of the pulsating subdwarf B eclipsing binary PG 1336 018 (NY Virginis)

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 Am binary systems in the SuperWASP survey

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- ...of spectroscopic binaries is 60 ∼ 70%. Thus, the eclipsing fraction appears to be ... See full document

20

A holistic study of the eclipsing binary EQ Tau

A holistic study of the eclipsing binary EQ Tau

... reliable spectroscopic elements of the system were estimated by Rucinski et ...published spectroscopic elements to yield the absolute parameters of the ...present analysis, Li et al. (2014) presents ... See full document

21

EG and: Far ultraviolet spectroscopic explorer and Hubble space telescope STIS monitoring of an eclipsing symbiotic binary

EG and: Far ultraviolet spectroscopic explorer and Hubble space telescope STIS monitoring of an eclipsing symbiotic binary

... our analysis of the P Cygni profiles and the radial velocity analysis of the unabsorbed broad lines, we can conclude that this material is located very close to the dwarf ...in-depth analysis of the ... See full document

12

A Wind analysis of an evolved Giant  FUSE and HST/STIS observations of an eclipsing Symbiotic Binary

A Wind analysis of an evolved Giant FUSE and HST/STIS observations of an eclipsing Symbiotic Binary

... of eclipsing symbiotic binary systems, containing a mass-losing giant and a hot white dwarf, are ideal for studying the wind generation mechanisms in evolved ... See full document

9

RZ COMAE – A W-TYPE OVERCONTACT ECLIPSING BINARY

RZ COMAE – A W-TYPE OVERCONTACT ECLIPSING BINARY

... UMa–type binary system, type–W, which has had, over the years, two spectroscopic and numerous light curve ...fresh analysis by the Wilson-Devinney 2003 ...period analysis attaining a LiTE ... See full document

23

A magnetic white dwarf in a detached eclipsing binary

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 ...and spectroscopic data for this ...Our ... 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

Eclipsing binaries observed with the WIRE satellite I, Discovery and photometric analysis of the new bright A0 IV eclipsing binary ψ Centauri

... detached eclipsing bi- nary system and as an object for a detailed asteroseismic ...SPB stars as determined from theory (Pamyatnykh 1999) may have to be extended towards the blue edge of the Cepheid insta- ... See full document

9

The EBLM project : II  A very hot, low mass M dwarf in an eccentric and long period, eclipsing binary system from the SuperWASP survey

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

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

Photometric Analysis of Eclipsing Binary Stars

Photometric Analysis of Eclipsing Binary Stars

... the binary components, we adjusted a numerical eclipsing binary model to the observations; the mass-ratio of CG Cyg and XY UMa were fixed at the values of ... See full document

10

COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS

COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS

... In this 77th compilation of BAV results, photoelectric observations obtained mostly in the years 2013 and 2014 are presented on 591 variable stars giving 962 minima on eclipsing binaries and maxima on ... See full document

17

On the dynamical stability of the proposed planetary system orbiting NSVS 14256825

On the dynamical stability of the proposed planetary system orbiting NSVS 14256825

... The intriguing possibility of circumbinary planets has been a fea- ture of science-fiction for decades. Theoretical studies of plane- tary formation have shown that such systems are indeed possible (Quintana & ... See full document

5

IBVS Volume 6101

IBVS Volume 6101

... In this 86th compilation of BAV results, photoelectric observations obtained mostly in the years 2015 and 2016 are presented on 1,063 variable stars giving 1,850 minima of eclipsing binaries. All moments of ... See full document

27

INFORMATION BULLETIN ON VARIABLE STARS

INFORMATION BULLETIN ON VARIABLE STARS

... CzeV615 – a New Eclipsing Binary . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1 – 6 6125 BAS¸T ¨ URK, ¨ O.; BAHAR, E.; S¸ENAVCI, H.V.; KILIC ¸ O ˘ GLU, T.; ¨ OZAVCI, ˙I.; ... See full document

13

Empirical isochrones and relative ages for young stars, and the radiative-convective gap

Empirical isochrones and relative ages for young stars, and the radiative-convective gap

... In addition, our comparison reveals three serious concerns. (i) Figs 18 and 21 show that whilst an acceptable fit to the theoretical isochrones can be obtained over most of the sequence, the model isochrone lies above ... See full document

22

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