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Stellar Surface Magneto-Convection as a Source of Astrophysical Noise. I. Multi-component Parameterisation of Absorption Line Profiles (2012)

First Author: Cegla H

Attributed to: The transient sky: an integrated programme of study 2011 - 2016 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1212.0236

Publication URI: https://arxiv.org/abs/1212.0236

Type: Other