(Q56080913)

English

Discovery of a brown dwarf in the Pleiades star cluster

scientific article published in Nature

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scholarly article

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Discovery of a brown dwarf in the Pleiades star cluster (English)

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María Rosa Zapatero Osorio

object named as

M. R. Zapatero Osorio

2

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author name string

R. Rebolo

1

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E. L. Martín

3

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language of work or name

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publication date

September 1995

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377

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6545

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129–131

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https://scigraph.springernature.com/pub.10.1038/377129a0

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An expanded set of brown dwarf and very low mass star models

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New pre-main-sequence tracks for M < 2.5 M as tests of opacities and convection model

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Luminosity functions for very low mass stars and brown dwarfs

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The solar neighborhood. II. The first list of dwarfs with spectral types of M7 and cooler

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Low mass companions to nearby stars: spectral classification and its relation to the stellar/substellar break

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The mass-luminosity relation for stars of mass 1.0 to 0.08 solar mass

1 reference

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A CCD-based search for very low mass members of the Pleiades cluster

1 reference

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Spectroscopy of a brown dwarf candidate in the alpha Persei open cluster

1 reference

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A spectroscopic test for substellar objects

1 reference

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Constraints to the masses of brown dwarf candidates from the lithium test

1 reference

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A search for lithium in Pleiades brown dwarf candidates using the Keck HIRES echelle

1 reference

https://api.crossref.org/works/10.1038%2F377129A0

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A search for low-mass stars and brown dwarfs in the Pleiades

1 reference

https://api.crossref.org/works/10.1038%2F377129A0

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based on heuristic

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Radial velocities of very low mass stars and candidate brown dwarf members of the Hyades and Pleiades. II

1 reference

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Radial velocities of very low mass stars and candidate brown dwarf members of the Hyades and Pleiades

1 reference

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Chromospheric and coronal activity of low-mass stars in the Pleiades

1 reference

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A search for substellar companions to low-mass stars

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The luminosity function at the end of the main sequence: results of a deep, large-area, CCD survey for cool dwarfs

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US naval observatory CCD parallaxes of faint stars. I. Program description and first results

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M dwarf spectra from O.6 to 1.5 microns: a spectral sequence, model atmosphere fitting and the temperature scale

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The faintest stars: infrared photometry, spectra, and bolometric magnitudes

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based on heuristic

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Optical spectroscopy of very low mass stars in the Pleiades

1 reference

https://api.crossref.org/works/10.1038%2F377129A0

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based on heuristic

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The search for faint members of the Pleiades. II. Colors, spectral types, and H-alpha emission line strengths for M dwarfs in the Pleiades, Hyades, and Gliese field

1 reference

https://api.crossref.org/works/10.1038%2F377129A0

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New evolutionary tracks for very low mass stars

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Identifiers

10.1038/377129A0

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1995Natur.377..129R

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