J. Farihi et al 2005 ApJ 627 L41 doi:10.1086/432158
J. Farihi1,2, P. R. Wood3 and B. Stalder4
Show affiliationsSpectroscopy and photometry demonstrate that SSSPM J1549-3544 is not a cool white dwarf, but a high-velocity metal-poor halo star.
stars: fundamental parameters; stars: individual (SSSPM J1549–3544); stars: kinematics; subdwarfs; white dwarfs
Issue 1 (2005 July 1)
Received 2005 April 22, accepted for publication 2005 May 25
Published 2005 June 10
J. Farihi et al 2005 ApJ 627 L41
N Bhargava Ram et al 2009 J. Phys. B: At. Mol. Opt. Phys. 42 225203
Sin Kim et al 2009 Meas. Sci. Technol. 20 125404
Hau-Wei Lee and Chieh-Li Chen 2009 Meas. Sci. Technol. 20 125103
Wen-Xing Yang et al 2009 J. Phys. B: At. Mol. Opt. Phys. 42 225501
J A Ludlow et al 2009 J. Phys. B: At. Mol. Opt. Phys. 42 225204
C P Malone et al 2009 J. Phys. B: At. Mol. Opt. Phys. 42 225202
F J Acevedo Rodriguez et al 2009 Meas. Sci. Technol. 20 125202
F Mohd-Yasin et al 2010 Meas. Sci. Technol. 21 012001
G S Buller and R J Collins 2010 Meas. Sci. Technol. 21 012002