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A dynamical calibration of the mass–luminosity relation at very low stellar masses and young ages

Author

Listed:
  • Laird M. Close

    (University of Arizona)

  • Rainer Lenzen

    (Max-Plank-Institut fur Astronomie)

  • Jose C. Guirado

    (Universitat de Valencia)

  • Eric L. Nielsen

    (University of Arizona)

  • Eric E. Mamajek

    (University of Arizona)

  • Wolfgang Brandner

    (Max-Plank-Institut fur Astronomie)

  • Markus Hartung

    (European Southern Observatory)

  • Chris Lidman

    (European Southern Observatory)

  • Beth Biller

    (University of Arizona)

Abstract

Star formation: evidence of mass The rapidly spinning young star AB Doradus (AB Dor) is thought to have a low-mass companion star, detected as an astrometric ‘wobble’. It has proved elusive — even to the Hubble Space Telescope — but now a new instrument built to image extrasolar planets shows what it can do by observing the faint companion. The high-contrast NACO SDI adaptive optics camera at the European Southern Observatory reveals the object, dubbed AB Dor C, to be of very low mass for a star (90 times that of Jupiter). It is 400 °C cooler and 2.5 times fainter than predicted by stellar models. This suggests that most known brown dwarfs and extrasolar planets are heavier than was thought, and the new findings will be important for the design of future cameras intended to find extrasolar planets. See the cover story for more on the search for new planets.

Suggested Citation

  • Laird M. Close & Rainer Lenzen & Jose C. Guirado & Eric L. Nielsen & Eric E. Mamajek & Wolfgang Brandner & Markus Hartung & Chris Lidman & Beth Biller, 2005. "A dynamical calibration of the mass–luminosity relation at very low stellar masses and young ages," Nature, Nature, vol. 433(7023), pages 286-289, January.
  • Handle: RePEc:nat:nature:v:433:y:2005:i:7023:d:10.1038_nature03225
    DOI: 10.1038/nature03225
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