activity
19972022
most citedThe Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data

848 citations · 14k across the 153 of their papers we have counts for

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astro-ph1998★ 64 cited

Rotation periods of late-type stars in the young open cluster IC 2602

Sydney A. Barnes, Sabatino Sofia, Charles F. Prosser +1

We present the results of a monitoring campaign aimed at deriving rotation periods for a representative sample of stars in the young (30 Myr) open cluster IC 2602. Rotation periods…

astro-ph1998

Brown Dwarfs

Ben R. Oppenheimer, S. R. Kulkarni, John R. Stauffer

After a discussion of the physical processes in brown dwarfs, we present a complete, precise definition of brown dwarfs and of planets inspired by the internal physics of objects b…

astro-ph1998

Discovery of a Very Low-Mass Binary with HST/NICMOS

E. L. Martin, G. Basri, W. Brandner +7

Hubble Space Telescope NICMOS observations are presented of six brown dwarf candidates in the Pleiades open cluster. One of them, namely CFHT-Pl-18, is clearly resolved as a binary…

astro-ph1998★ 29 cited

Stellar Activity in Coeval Open Clusters: Praesepe and The Hyades

D. Barrado y Navascues, J. R. Stauffer, S. Randich

Randich and Schmitt [1995, A&A 298, 115] found that the coronal activity of solar-type and low mass stars in Praesepe is significantly lower than that of stars in the Hyades cluste…

astro-ph1998★ 455 cited

Keck Spectra of Pleiades Brown Dwarf Candidates and a Precise Determination of the Lithium Depletion Edge in the Pleiades

John Stauffer, Greg Schultz, J. Davy Kirkpatrick

We have obtained intermediate resolution spectra of eleven candidate brown dwarf members of the Pleiades open cluster using the Keck II telescope and LRIS spectrograph. Our primary…

astro-ph1998★ 232 cited

The Problem of Hipparcos Distances to Open Clusters: I. Constraints from Multicolor Main Sequence Fitting

Marc H. Pinsonneault, John Stauffer, David R. Soderblom +2

Parallax data from the Hipparcos mission allow the direct distance to open clusters to be compared with the distance inferred from main sequence (MS) fitting. There are surprising…