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
Jeroen P van der Sluijs et al 2008 Environ. Res. Lett. 3 024008
Zhiping Xu and Markus J Buehler 2009 Nanotechnology 20 375704
J Kubler et al 1988 J. Phys. F: Met. Phys. 18 469
Carlos Alves et al 2009 Inverse Problems 25 055005
Rainer Kress and Pedro Serranho 2005 Inverse Problems 21 773
Pedro Serranho 2006 Inverse Problems 22 663
Renzhi Lu et al 2008 Phys. Med. Biol. 53 6749
Renzhi Lu et al 2007 Phys. Med. Biol. 52 849
N M R Peres and Ricardo M Ribeiro 2009 New J. Phys. 11 095002