Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458
- I. Baraffe, G. Chabrier, T. Allard, P. Hauschildt
- Physics
- 14 February 2003
We present evolutionary models for cool brown dwarfs and extra-solar giant planets. The models re- produce the main trends of observed methane dwarfs in near-IR color-magnitude diagrams. We also… Expand
Evolutionary Models for Very Low-Mass Stars and Brown Dwarfs with Dusty Atmospheres
- G. Chabrier, I. Baraffe, F. Allard, P. Hauschildt
- Physics
- 29 May 2000
We present evolutionary calculations for very low-mass stars and brown dwarfs based on synthetic spectra and nongray atmosphere models which include dust formation and opacity, i.e., objects with… Expand
LOW-TEMPERATURE OPACITIES
- J. Ferguson, D. Alexander, +5 authors A. Tamanai
- Physics
- 2 February 2005
Previous computations of low-temperature Rosseland and Planck mean opacities from Alexander & Ferguson areupdatedandexpanded.Thenewcomputationsincludeamorecompleteequationofstate(EOS)withmoregrain… Expand
A new extensive library of PHOENIX stellar atmospheres and synthetic spectra
- T. Husser, S. Berg, +4 authors P. Hauschildt
- Physics
- 22 March 2013
Aims. We present a new library of high-resolution synthetic spectra based on the stellar atmosphere code PHOENIX that can be used for a wide range of applications of spectral analysis and stellar… Expand
The NEXTGEN Model Atmosphere Grid. II. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 K
- P. Hauschildt, F. Allard, J. Ferguson, Eddie Baron, D. Alexander
- Physics
- 14 July 1999
We present the extension of our NextGen model atmosphere grid to the regime of giant stars. The input physics of the models presented here is nearly identical to that of the NextGen dwarf atmosphere… Expand
Infrared Spectra and Spectral Energy Distributions of Late M and L Dwarfs
- S. Leggett, F. Allard, T. Geballe, P. Hauschildt, A. Schweitzer
- Physics
- 10 October 2000
We have obtained 1.0-2.5 ?m spectra at R ~ 600 of 14 disk dwarfs with spectral types M6-L7. For four of the dwarfs, we have also obtained infrared spectra at R ~ 3000 in several narrow intervals. In… Expand
Infrared Spectra of Low-Mass Stars: Toward a Temperature Scale for Red Dwarfs
- S. Leggett, F. Allard, G. Berriman, C. C. Dahn, P. Hauschildt
- Physics
- 1 May 1996
We present new low-resolution (R ~ 250) 1.0-2.4 pm spectra for 13 red dwarf stars. The sample size is increased to 16 by including other published infrared spectra. New, as well as published, red… Expand
Evidence for a Spectroscopic Sequence among Type Ia Supernovae
- P. Nugent, M. Phillips, Eddie Baron, D. Branch, P. Hauschildt
- Physics
- 2 October 1995
In this Letter we present evidence for a spectral sequence among Type Ia supernovae (SN Ia's). The sequence is based on the systematic variation of several features seen in the near-maximum light… Expand
The M Dwarf GJ 436 and its Neptune-Mass Planet
We determine stellar parameters for the M dwarf GJ 436, which hosts a Neptune-mass planet. We employ primarily spectral modeling at low and high resolution, examining the agreement between model and… Expand
An Effective Temperature Scale for Late-M and L Dwarfs, from Resonance Absorption Lines of Cs I and Rb I
- G. Basri, S. Mohanty, +5 authors B. Goldman
- Physics
- 2 March 2000
We present Keck HIRES spectra of six late-M dwarfs and 11 L dwarfs. Our goal is to assign effective temperatures to the objects using detailed atmospheric models and fine analysis of the alkali… Expand