dc.contributor.author | Pravdo, Steven H. | en_US |
dc.contributor.author | Angelini, Lorella | en_US |
dc.contributor.author | Shaklan, Stuart B. | en_US |
dc.date.accessioned | 2004-09-29T22:29:37Z | |
dc.date.available | 2004-09-29T22:29:37Z | |
dc.date.issued | 1996 | en_US |
dc.identifier.clearanceno | 96-0077 | en_US |
dc.identifier.uri | http://hdl.handle.net/2014/23632 | |
dc.description.abstract | We have identified three new weak lined T Tauri stars in Orion using the Double Spectrograph and 5-m telescope at Palomar Observatory. One of these is a candidate for the X-ray source RX0535-0633. H(alpha) and H(beta) line emisison are detected and equivalent widths measured in all three stars, and in V942 Ori. We also searched without success for H(alpha) line variability in V942 Ari. | en_US |
dc.format.extent | 396620 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.subject.other | stars emission line be stars flare stars V942 Ori V942 Ari Orion | en_US |
dc.title | Three Weak-Lined T Tauri Stars in Orion | en_US |