The shortest period M dwarf eclipsing system BW3 V38 II. Determination of absolute elements

Astronomy and Astrophysics

Volumn 426, Issue 2, 2004, Pages 577-585

  Maceroni, C ^a   Montalban J ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^b UNIVERSITY OF LIÈGE   (Belgium)

Author keywords

Stars: binaries: close; Stars: binaries: eclipsing; Stars: fundamental parameters; Stars: individuals: OGLE BW3 V38; Stars: late type

Indexed keywords

DATA REDUCTION; ERRORS; MAGNETIC FIELD EFFECTS; MICROLENSES; OPTICAL RESOLVING POWER; ORBITS; PHOTOMETRY; SPECTROSCOPIC ANALYSIS;

BINARIES; CHROMOSPHERES; FUNDAMENTAL PARAMETERS; STARS;

ASTROPHYSICS;

EID: 8344242180     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040549     Document Type: Article

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