[PDF] Top 20 ANOTHER COMPONENT IN THE V523 CASSIOPEIAE ECLIPSING BINARY SYSTEM
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ANOTHER COMPONENT IN THE V523 CASSIOPEIAE ECLIPSING BINARY SYSTEM
... with V ∼ 10 . 9 magnitudes and about 1.0 magnitude difference between minimum and maximum. The system was observed using the Pisgah Astronomical Research Institute 0.4-m telescope equipped with an Apogee E42 ... See full document
6
SDSS J0926+3624 : the shortest period eclipsing binary star
... dominant component in the light curve is the primary white dwarf, and the main eclipse in the light curve is the eclipse of this ...this system: in higher mass ratio systems we would expect to see the ... See full document
20
Absolute Properties of the Low-Mass Eclipsing Binary CM Draconis
... continuities resulting from the more than 30 leap seconds that have been introduced in the interval spanned by the various data sets. For the anal- ysis in this section we used the 2005 version of the 2003 WD code ... See full document
20
Spectroscopic Analysis of Eclipsing Binary Stars
... short-period eclipsing binary system BX And on five nights in 1976 at the Morgan Monroe station of the Goethe link Observatory of Indiana ...And binary system consists of an F type ... See full document
8
TIMES OF MINIMA OF 116 ECLIPSING BINARY SYSTEMS (2010-2015)
... V471 Cas 56173.3973 0.0005 2 C AA30 V473 Cas 56175.3776 0.0006 1 C AA30 V523 Cas 54437.3404 0.0001 2 C AA30 V821 Cas 55588.2921 0.0001 1 V Pan26 V1031 Cas 56195.3611 0.0004 1 C AA30 V1107 Cas 56168.2899 0.0003 1 C ... See full document
7
A holistic study of the eclipsing binary EQ Tau
... primary component and only one on the secondary, also the more massive component is hotter than the low massive one by ∆T ~ 100 ...the system EQ Tau was constructed using the software package ... See full document
21
A magnetic white dwarf in a detached eclipsing binary
... the eclipsing PCEB SDSS J0303 + 0054 is a magnetic WD with a field strength of 8 MG, measured from Zeeman emission ...the system without the need for a circumbinary ... See full document
12
A magnetic white dwarf in a detached eclipsing binary
... The average spectrum of SDSS J0303+0054 is shown in Figure 5. The two components are easily visible, although no absorption fea- tures from the white dwarf are detected, confirming its DC nature. Several strong emission ... See full document
15
A New Detached M Dwarf Eclipsing Binary
... Our original (unrectified) photometric light curve contains nonuniform out-of-eclipse variations. Binary systems such as TrES-Her0-07621 are often magnetically active (e.g., Strassmeier et al. 1993). While tidal ... See full document
5
Doppler images of the eclipsing binary ER Vulpeculae
... close binary systems like ER ...both component stars in the close binaries are magnetic connecting, and the active longitude belts are related to the interac- tion between magnetic ...CVn-type binary ... See full document
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The EBLM project : II A very hot, low mass M dwarf in an eccentric and long period, eclipsing binary system from the SuperWASP survey
... metal-poor system, as determined by the large radius and the spectrum of the solar-type primary star with an eccentric and long-period ...the eclipsing binary model, the stellar characterisation of ... See full document
13
Blend Analysis of HATNet Transit Candidates
... by another star, or by a non-luminous object (planet or brown ...the eclipsing system and the eccentricity and argument of periastron are input into ebop (Popper & Etzel 1981; Etzel 1981; Nelson ... See full document
6
HATS-31b through HATS-35b: five transiting hot Jupiters discovered by the HATSouth survey
... stellar binary false positives and con fi rm planetary candidates detected by the HATSouth network, we carry out initial low- and medium-resolution reconnaissance spectroscopy before attempting higher precision ... See full document
16
The binary properties of the pulsating subdwarf B eclipsing binary PG 1336 018 (NY Virginis)
... a binary fraction of 40% among stars in the SPY (Supernova type Ia Progenitor) survey sample, while Morales-Rueda et ...the binary sdBs are found to be in short period systems with periods from a few hours ... See full document
12
NEW LIGHT-TIME CURVE OF ECLIPSING BINARY AM Leo
... the eclipsing binary AM Leo generally between 1996–2017 at Kourovka Astronomical Observatory of the Ural Federal University in Russia, which have not been published ... See full document
6
KIC 2856960 : the impossible triple star
... close binary in the left two panels (solid) and star 3 in the left- and right-hand panels ...second binary formed from star 3, the star that is eclipsed during the dips, and an extra star, “star 4”, ... See full document
12
USING APASS STANDARDS TO TRANSFORM CCD OBSERVATIONS:
... standard system, they also enable the re- analysis of existing observations to transform them as well, even in the case where the existing observations were made in only one ... See full document
6
The substellar companion in the eclipsing white dwarf binary SDSS J141126.20+200911.1
... VSD, SPL and ULTRACAM are supported by STFC grant ST/J001589/1. TRM and SC are supported by STFC grant ST/L000733/1. TRM and MCP acknowledge the support of the International Exchange Scheme from the Royal Astro- nomical ... See full document
12
TIMES OF MINIMA OF SOME ECLIPSING BINARY STARS WITH ECCENTRIC MINIMA IN THE KEPLER FIELD II.
... This paper is a continuation of the work published in IBVS 6219 (Bulut, 2017). In this study, we present 1086 minima times of 6 eclipsing binaries with eccentric orbit. The eclipse-timing variation O–C curves of ... See full document
27
GSC 02996-00858: A NEW ALGOL-TYPE ECLIPSING BINARY IN LEO
... V = 14.48) was followed over six nights and confirmed to be an eclipsing binary with a deep primary minimum and a shallow secondary minimum. Perhaps of greater interest is the unexpected flare-like event ... See full document
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