HD 174884: A strongly eccentric, short-period early-type binary system discovered by CoRoT

Astronomy and Astrophysics

Volumn 508, Issue 3, 2009, Pages 1375-1389

  MacEroni, C ^a   Montalban J ^b   Michel, E ^c   Harmanec, P ^d   Prsa, A ^e,f   Briquet, M ^g   Niemczura, E ^g,h   Morel, T ^b,g   Ladjal, D ^g   Auvergne, M ^c   Baglin, A ^c   Baudin, F ^b   Catala, C ^c   Samadi, R ^c   Aerts, C ^g,i  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c OBSERVATOIRE DE PARIS   (France)

^d CHARLES UNIVERSITY   (Czech Republic)

^e VILLANOVA UNIVERSITY   (United States)

^f UNIVERSITY OF LJUBLJANA   (Slovenia)

^g UNIVERSITY OF LEUVEN   (Belgium)

^h UNIVERSITY OF WROC AW   (Poland)

ⁱ RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

Author keywords

Binaries: close; Binaries: eclipsing; Stars: fundamental parameters; Stars: individual: HD 174884; Stars: variables: general

Indexed keywords

BINARIES: CLOSE; BINARIES:ECLIPSING; BINARY SYSTEMS; BOOTSTRAP RESAMPLING; DEPTH RATIO; ECCENTRIC ORBITS; FITTING MODEL; FOLLOW-UP PROGRAMS; HIGH DISPERSION; LEVENBERG-MARQUARDT MINIMIZATION; LIGHT CURVES; ORBITAL FREQUENCIES; ORBITAL PERIODS; PASS BANDS; RADIAL VELOCITY CURVES; SECONDARY ECLIPSE; SIMULTANEOUS FITTING; SOLUTION UNIQUENESS; SPACE OBSERVATIONS; SPECTROSCOPIC BINARY; STARS: INDIVIDUAL; STARS: VARIABLES: GENERAL; SYNCHRONOUS COMPONENTS; THEORETICAL MODELS; TWO-COMPONENT; BINARIES: ECLIPSING; STARS: FUNDAMENTAL PARAMETERS; STARS: INDIVIDUAL: HD 174884;

CURVE FITTING; FOURIER ANALYSIS; ORBITS; PHOTOMETRY;

STARS;

EID: 72849127066     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913311     Document Type: Article

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