Prospects for observing pulsating red giants with the MONS Star Trackers

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dc.creatorBedding, Timothy R.
dc.date2000-03-17
dc.date.accessioned2026-07-07T01:52:47Z
dc.date.available2026-07-07T01:52:47Z
dc.descriptionK and M giants show variability on timescales from years down to days and possibly even hours. I discuss the contribution that can be made with high-precision photometry that will be obtained by the MONS Star Trackers. These include observations of flare-like events on Mira variables, and oscillation spectra for K giants and short-period M giants.
dc.description5 pages, LaTeX, 2 Postscript figures. To appear in Proceedings of the Third MONS Workshop: Science Preparation and Target Selection, edited by T.C.V.S. Teixeira and T.R. Bedding (Aarhus: Aarhus Universitet)
dc.identifierhttps://arxiv.org/abs/astro-ph/0003250
dc.identifierhttp://arxiv.org/abs/astro-ph/0003250
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/738
dc.subjectAstrophysics
dc.titleProspects for observing pulsating red giants with the MONS Star Trackers
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