VLTI observations of IRS~3: The brightest compact MIR source at the Galactic Centre

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dc.creatorPott, J. -U.
dc.creatorEckart, A.
dc.creatorGlindemann, A.
dc.creatorViehmann, T.
dc.creatorSchödel, R.
dc.creatorStraubmeier, C.
dc.creatorLeinert, C.
dc.creatorFeldt, M.
dc.creatorGenzel, R.
dc.creatorRobberto, M.
dc.date2005-05-10
dc.date.accessioned2026-07-07T02:17:36Z
dc.date.available2026-07-07T02:17:36Z
dc.descriptionThe dust enshrouded star IRS~3 in the central light year of our galaxy was partially resolved in a recent VLTI experiment. The presented observation is the first step in investigating both IRS~3 in particular and the stellar population of the Galactic Centre in general with the VLTI at highest angular resolution. We will outline which scientific issues can be addressed by a complete MIDI dataset on IRS~3 in the mid infrared.
dc.description4 pages, 3 figures, published in: The ESO Messenger
dc.identifierhttps://arxiv.org/abs/astro-ph/0505189
dc.identifierhttp://arxiv.org/abs/astro-ph/0505189
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9228
dc.subjectAstrophysics
dc.titleVLTI observations of IRS~3: The brightest compact MIR source at the Galactic Centre
dc.typetext

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