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

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

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_67366706

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

About this item

Full title

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

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2005-01, Vol.433 (7023), p.286-289

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

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...

Alternative Titles

Full title

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

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_67366706

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_67366706

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/nature03225

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