The nearest cool white dwarf (d ∼ 4 pc), the coolest M-type subdwarf (sdM9.5), and other high proper motion discoveries

Astronomy and Astrophysics

Volumn 425, Issue 2, 2004, Pages 519-527

  Scholz, R D ^a   Lehmann, I ^b   Matute, I ^b   Zinnecker, H ^a  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Astrometry; Stars: kinematics; Stars: low mass, brown dwarfs; Stars: subdwarfs; Stars: white dwarfs; Surveys

Indexed keywords

DISKS (STRUCTURAL COMPONENTS); INFRARED SPECTROSCOPY; KINEMATICS; PHOTOMETRY; SAMPLING; SOLAR SYSTEM;

ASTROMETRY; BROWN DWARFS; STARS: KINEMATICS; STARS: LOW MASS; STARS: SUBDWARFS; STARS: WHITE DWARFS;

GALAXIES;

EID: 5044245739     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041059     Document Type: Article

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