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astro-phMay 26, 2005
6
citations (OpenAlex)
authors
  • J. Farihi
  • P. R. Wood
  • B. Stalder
institutions
  • Australian National University
  • International Gemini Observatory
  • University of California, Los Angeles
  • University of Hawaiʻi at Mānoa
  • University of Hawaii System
arXiv abstractPDF
paper

SSSPM J1549−3544 Is Not a White Dwarf

arXiv:astro-ph/0505525 · doi:10.1086/432158

Abstract

Spectroscopy and photometry demonstrate that SSSPM J1549−3544 is not a cool white dwarf but a high velocity metal-poor halo star.

8 pages, 1 figure, 2 tables, accepted to ApJ Letters

References in corpus (4)

  • A Catalog of Northern Stars With Annual Proper Motions Larger Than 0.15 Seconds of Arc (LSPM catalog - North)
  • The nearest cool white dwarf (d~4pc), the coolest M-type subdwarf (sdM9.5), and other high proper motion discoveries
  • Photometric Identification of Cool White Dwarfs
  • Cool Versus Ultracool White Dwarfs

Cited by in corpus (5)

  • Optical spectroscopy of high proper motion stars: new M dwarfs within 10 pc and the closest pair of subdwarfs
  • Spectroscopic distances of 28 nearby star candidates
  • One of Everything: The Breakthrough Listen Exotica Catalog
  • Spectroscopic classification and Gaia DR2 parallaxes of new nearby white dwarfs among selected blue proper motion stars
  • 2MASS J06562998+3002455: Not a Cool White Dwarf Candidate, but a Population II Halo Star
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