The Nature of the Variable Galactic Center Source IRS16SW

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dc.creatorDePoy, D. L.
dc.creatorPepper, J.
dc.creatorPogge, Richard W.
dc.creatorStutz, Amelia
dc.creatorPinsonneault, M.
dc.creatorSellgren, K.
dc.date2004-08-30
dc.date.accessioned2026-07-07T13:14:11Z
dc.date.available2026-07-07T13:14:11Z
dc.descriptionWe report measurements of the light curve of the variable Galactic Center source IRS16SW. The light curve is not consistent with an eclipsing binary or any other obvious variable star. The source may be an example of a high mass variable predicted theoretically but not observed previously.
dc.description11 pages, 2 figures. Accepted by ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0408561
dc.identifierhttp://arxiv.org/abs/astro-ph/0408561
dc.identifierAstrophys.J.617:1127-1130,2004
dc.identifierdoi:10.1086/425557
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230131
dc.subjectAstrophysics
dc.titleThe Nature of the Variable Galactic Center Source IRS16SW
dc.typetext

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