The mass-luminosity relation for stars of mass 1.0 to 0.08script M sign

Todd J. Henry, Donald W. Mccarthy

Research output: Contribution to journalArticlepeer-review

371 Scopus citations

Abstract

Mass-luminosity relations determined at infrared wavelengths are presented for stars with masses 1.0 to 0.08script M sign. Using infrared speckle imaging techniques on a sample of nearby binaries, we have been able to concentrate on the lower main sequence (script M sign≤0.5script M sign), for which an accurate mass-luminosity calibration has remained problematic. In addition, the mass-visual luminosity relation for stars with 20≥scriptMsign≥0.08script M sign is produced by implementing new photometric relations linking V to JHK wavelengths for the nearby stars, supplemented with eclipsing binary information. These relations predict that objects with masses ∼0.08script M sign have MK∼10 and MV∼18.

Original languageEnglish (US)
Pages (from-to)773-789
Number of pages17
JournalAstronomical Journal
Volume106
Issue number2
DOIs
StatePublished - Aug 1993

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'The mass-luminosity relation for stars of mass 1.0 to 0.08script M sign<sub>⊙</sub>'. Together they form a unique fingerprint.

Cite this