Hostname: page-component-745bb68f8f-f46jp Total loading time: 0 Render date: 2025-02-03T14:46:01.688Z Has data issue: false hasContentIssue false
  • English
  • Français

The MONS/Rømer Experiment

Published online by Cambridge University Press:  12 April 2016

H. Kjeldsen
H. Kjeldsen*
Affiliation:
Teoretisk Astrofysik Center andInstitut for Fysik og Astronomi, Aarhus Universitet, DK-8000 Aarhus C, Denmark. email: hans@ifa.au.dk

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The aim of the MONS (Measuring Oscillations in Nearby Stars) project is to use observations of stellar oscillations to perform an asteroseismic analysis of stellar interiors. We expect to obtain high precision oscillation measurements on a sample of 20 bright stars as well as oscillation data at a slightly lower level of precision, but on a larger sample of bright stars. MONS will be launched on the Danish Rømer satellite in mid 2005.

Type
Part 6. Asteroseismology from Space and from the Ground
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 630 - 633
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Christensen-Dalsgaard, J. 2001, in Proc. 1st Eddington workshop, eds. Favata, F., Roxburgh, I.W. & Galadi, D., ESA SP-485, in pressGoogle Scholar