Radio emission from RASS sources south of Taurus-Auriga

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dc.creatorMagazzu, A.
dc.creatorUmana, G.
dc.creatorMartin, E. L.
dc.date1999-03-09
dc.date.accessioned2026-07-07T02:30:44Z
dc.date.available2026-07-07T02:30:44Z
dc.descriptionWe present a 8.4 GHz VLA survey of 50 optical counterparts to 46 ROSAT All-Sky survey (RASS) X-ray sources south of the Taurus-Auriga star-forming region. This survey detected 3 sources with a sensitivity limit of ~ 0.12 mJy. Merging our sample with other radio observations of sources in and around Taurus-Auriga, we find scarce radio emission among RASS sources south of the Taurus-Auriga molecular clouds. Our data support the evidence that these sources are older than weak-lined T Tauri stars, most of them probably being close to the ZAMS.
dc.description6 pages, 2 figures, aa.cls LaTeX class
dc.identifierhttps://arxiv.org/abs/astro-ph/9903125
dc.identifierhttp://arxiv.org/abs/astro-ph/9903125
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13915
dc.subjectAstrophysics
dc.titleRadio emission from RASS sources south of Taurus-Auriga
dc.typetext

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