Synthetic pulsational line profile variations

Oreiro R, Telting JH, Ostensen RH, Briquet M, Aerts C, Heber U, Heber U, Vuckovic M (2010)

Publication Status: Published

Publication Type: Journal article

Publication year: 2010

Journal

Astrophysics and Space Science Springer Verlag (Germany)

Publisher: SPRINGER

Book Volume: 329

Pages Range: 211-216

Journal Issue: 1-2

DOI: 10.1007/s10509-010-0415-x

Abstract

We have produced simulated time series of high resolution spectroscopy for sdBs. We present the first results of testing classical mode identification techniques. Here, in particular, we analyse the behaviour of individual spectral lines and discuss the results and applicability of the moment method.

Authors with CRIS profile

Ulrich Heber Professur für Astronomie und Astrophysik

Involved external institutions

Katholieke Universiteit Leuven (KUL) / Catholic University of Leuven BE Belgium (BE) Roque de los Muchachos Observatory / Observatorio del Roque de los Muchachos (ORM) ES Spain (ES)

How to cite

APA:

Oreiro, R., Telting, J.H., Ostensen, R.H., Briquet, M., Aerts, C., Heber, U.,... Vuckovic, M. (2010). Synthetic pulsational line profile variations. Astrophysics and Space Science, 329(1-2), 211-216. https://doi.org/10.1007/s10509-010-0415-x

MLA:

Oreiro, R., et al. "Synthetic pulsational line profile variations." Astrophysics and Space Science 329.1-2 (2010): 211-216.

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