Mass-radius relation of low and very low-mass stars revisited with the VLTI

Astronomy and Astrophysics

Volumn 505, Issue 1, 2009, Pages 205-215

  Demory, B O ^a   Segransan D ^a   Forveille, T ^b   Queloz, D ^a   Beuzit, J L ^b   Delfosse, X ^b   Di Folco, E ^a,c   Kervella, P ^c   Le Bouquin, J B ^d   Perrier, C ^b   Benisty, M ^e   Duvert, G ^b   Hofmann, K H ^f   Lopez, B ^g   Petrov, R ^h  

^a UNIVERSITÉ DE GENÈVE   (Switzerland)

^b LABORATOIRE D ASTROPHYSIQUE   (France)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^f MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^g UNIVERSITÉ CÔTE D'AZUR   (France)

^h UNIVERSITÉ DE NICE SOPHIA ANTIPOLIS   (France)

Author keywords

Stars: fundamental parameters; Stars: low mass, brown dwarfs; Techniques: interferometric

Indexed keywords

ECLIPSING BINARIES; LONG-BASELINE INTERFEROMETRY; LOW-MASS STARS; MAGNETIC ACTIVITY; MIXING LENGTH; NEAR INFRARED; RECOMBINERS; STARS: FUNDAMENTAL PARAMETERS; STARS: LOW-MASS, BROWN DWARFS; STELLAR EVOLUTIONS; TECHNIQUES: INTERFEROMETRIC;

INTERFEROMETERS; INTERFEROMETRY; LUMINANCE; OPTICAL TELESCOPES;

STARS;

EID: 70349678837     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911976     Document Type: Article

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