Evidence for Early Circumstellar Disk Evolution in NGC 2068/71

dc.creatorFlaherty, K. M.
dc.creatorMuzerolle, J.
dc.date2007-12-10
dc.date.accessioned2026-07-07T12:24:05Z
dc.date.available2026-07-07T12:24:05Z
dc.descriptionWe study the disk and accretion properties of young stars in the NGC 2068 and NGC 2071 clusters. Using low-resolution optical spectra, we define a membership sample and determine an age for the region of ~2 Myr. Using high-resolution spectra of the H-alpha line we study the accretion activity of these likely members and also examine the disk properties of the likely members using IRAC and MIPS mid-infrared photometry. A substantial fraction (79%) of the 67 members have an infrared excess while all of the stars with significant infrared excess show evidence for active accretion. We find three populations of evolved disks (IRAC-weak, MIPS-weak and transition disks) all of which show decreased accretion activity in addition to the evidence for evolution in the dust disk.
dc.description44 pages (20 pages of text), 16 figures, 5 tables
dc.identifierhttps://arxiv.org/abs/0712.1601
dc.identifierhttp://arxiv.org/abs/0712.1601
dc.identifierAstron.J.135:966-983,2008
dc.identifierdoi:10.1088/0004-6256/135/3/966
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/214210
dc.subjectAstrophysics
dc.titleEvidence for Early Circumstellar Disk Evolution in NGC 2068/71
dc.typetext

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