The StaggerGrid project: a grid of 3-D model atmospheres for high-precision spectroscopy

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Standard

The StaggerGrid project : a grid of 3-D model atmospheres for high-precision spectroscopy. / Collet, Remo; Magic, Zazralt; Asplund, Martin.

I: Journal of Physics: Conference Series, Bind 328, Nr. 1, 012003, 2011.

Publikation: Bidrag til tidsskrift › Konferenceartikel › Forskning › fagfællebedømt

Harvard

Collet, R, Magic, Z & Asplund, M 2011, 'The StaggerGrid project: a grid of 3-D model atmospheres for high-precision spectroscopy', Journal of Physics: Conference Series, bind 328, nr. 1, 012003. https://doi.org/10.1088/1742-6596/328/1/012003

APA

Collet, R., Magic, Z., & Asplund, M. (2011). The StaggerGrid project: a grid of 3-D model atmospheres for high-precision spectroscopy. Journal of Physics: Conference Series, 328(1), [012003]. https://doi.org/10.1088/1742-6596/328/1/012003

Vancouver

Collet R, Magic Z, Asplund M. The StaggerGrid project: a grid of 3-D model atmospheres for high-precision spectroscopy. Journal of Physics: Conference Series. 2011;328(1). 012003. https://doi.org/10.1088/1742-6596/328/1/012003

Author

Collet, Remo ; Magic, Zazralt ; Asplund, Martin. / The StaggerGrid project : a grid of 3-D model atmospheres for high-precision spectroscopy. I: Journal of Physics: Conference Series. 2011 ; Bind 328, Nr. 1.

Bibtex

@inproceedings{9fa8b0459af74bf391c28da76606d5f8,
title = "The StaggerGrid project: a grid of 3-D model atmospheres for high-precision spectroscopy",
abstract = "In this contribution, we present the STAGGERGRID, a collaborative project for the construction of a comprehensive grid of time-dependent, three-dimensional (3-D), hydrodynamic model atmospheres of solar- and late-type stars with different effective temperatures, surface gravities, and chemical compositions. We illustrate the main characteristics of these 3-D models and their effects on the predicted strengths, wavelength-shifts, and shapes of spectral lines, highlighting the differences with respect to calculations based on classical, one-dimensional, hydrostatic models, and discuss some of their possible applications to elemental abundance analysis of stellar spectra in the context of large observational surveys.",
author = "Remo Collet and Zazralt Magic and Martin Asplund",
year = "2011",
doi = "10.1088/1742-6596/328/1/012003",
language = "English",
volume = "328",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "Institute of Physics Publishing Ltd",
number = "1",
note = "null ; Conference date: 23-06-2011 Through 24-06-2011",

}

RIS

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T1 - The StaggerGrid project

AU - Collet, Remo

AU - Magic, Zazralt

AU - Asplund, Martin

PY - 2011

Y1 - 2011

N2 - In this contribution, we present the STAGGERGRID, a collaborative project for the construction of a comprehensive grid of time-dependent, three-dimensional (3-D), hydrodynamic model atmospheres of solar- and late-type stars with different effective temperatures, surface gravities, and chemical compositions. We illustrate the main characteristics of these 3-D models and their effects on the predicted strengths, wavelength-shifts, and shapes of spectral lines, highlighting the differences with respect to calculations based on classical, one-dimensional, hydrostatic models, and discuss some of their possible applications to elemental abundance analysis of stellar spectra in the context of large observational surveys.

AB - In this contribution, we present the STAGGERGRID, a collaborative project for the construction of a comprehensive grid of time-dependent, three-dimensional (3-D), hydrodynamic model atmospheres of solar- and late-type stars with different effective temperatures, surface gravities, and chemical compositions. We illustrate the main characteristics of these 3-D models and their effects on the predicted strengths, wavelength-shifts, and shapes of spectral lines, highlighting the differences with respect to calculations based on classical, one-dimensional, hydrostatic models, and discuss some of their possible applications to elemental abundance analysis of stellar spectra in the context of large observational surveys.

UR - http://www.scopus.com/inward/record.url?scp=84856661248&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/328/1/012003

DO - 10.1088/1742-6596/328/1/012003

M3 - Conference article

AN - SCOPUS:84856661248

VL - 328

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012003

Y2 - 23 June 2011 through 24 June 2011

ER -

ID: 182329265