Determining the abundance of extragalactic planets

Simple item page
dc.creatorDominik, M.
dc.date2003-09-23
dc.date2003-10-23
dc.date.accessioned2026-07-07T02:09:43Z
dc.date.available2026-07-07T02:09:43Z
dc.descriptionGravitational microlensing provides a unique technique to reveal information about extragalactic planets. A network of at least four 2m-class telescopes distributed around the northern hemisphere could probe 15-35 jupiters and 4-10 saturns around M31 stars per year.
dc.description2 pages, LaTeX using newpasp.sty (supplied). To appear in the proceedings of the XIXth IAP colloquium "Extrasolar Planets: Today and Tomorrow" held in Paris, France, 2003 June 30 -- July 4, ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/0309607
dc.identifierhttp://arxiv.org/abs/astro-ph/0309607
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6537
dc.subjectAstrophysics
dc.titleDetermining the abundance of extragalactic planets
dc.typetext

Files

Collections

arXiv