Microlensing and the Physics of Stellar Atmospheres

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dc.creatorSackett, Penny D.
dc.date2000-04-17
dc.date.accessioned2026-07-07T01:53:11Z
dc.date.available2026-07-07T01:53:11Z
dc.descriptionThe simple physics of microlensing provides a well-understood tool with which to probe the atmospheres of distant stars in the Galaxy and Local Group with high magnification and resolution. Recent results in measuring stellar surface structure through broad band photometry and spectroscopy of high amplification microlensing events are reviewed, with emphasis on the dramatic expectations for future contributions of microlensing to the field of stellar atmospheres.
dc.description8 pages including 6 figures. To appear in ``Microlensing 2000: A New Era of Microlensing Astrophysics,'' an ASP conference proceedings, eds. J.W. Menzies and P.D. Sackett
dc.identifierhttps://arxiv.org/abs/astro-ph/0004237
dc.identifierhttp://arxiv.org/abs/astro-ph/0004237
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/877
dc.subjectAstrophysics
dc.titleMicrolensing and the Physics of Stellar Atmospheres
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