Terrestrial planets around M dwarfs via precise radial velocities. VLT+UVES observations of barnard's star = GJ 699

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 539, 2003, Pages 485-489

  Kürster, Martin ^a   Endl, Michael ^b   Rouesnel, Frederic ^c   Els, Sebastian ^d   Kaufer, Andreas ^e   Brillant, Stephane ^e   Hatzes, Artie P ^a   Saar, Steven H ^f   Cochran, William D ^b  

^a Thuringer L Tautenburg   (Germany)

^b Section of Molecular Genetics and Microbiology   (United States)

^c UNIVERSITÉ PARIS SACLAY   (France)

^d ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^e EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Extrasolar planets; Habitable zone; M dwarfs; Terrestrial planets

Indexed keywords

ACCELERATION; DATA REDUCTION; MATHEMATICAL MODELS; PLANETS; VELOCITY MEASUREMENT; WHITE NOISE;

EXTRASOLAR PLANETS; HABITABLE ZONES (HZ); M DWARFS; TERRESTRIAL PLANETS;

ASTRONOMY;

EID: 3142736011     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

References (6)

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2. Kürster M., Schmitt J.H.M.M., Cutispoto G., Dennerl K., 1997, A&A 320, 831
3. Benedict G.F., McArthur B., Chappel D.W. et al., 1999, AJ 118, 1086
4. Kürster M., Endl., Rouesnel et al., 2003, A&A, in press
5. Dobson A.K., Donahue R.A., Radick R.R., Kadlec K.L., 1990, ASP Conf. Str., Vol. 9, 132
6. Endl M., Kürster M., & Els S., 2000, A&A 362, 585