T Tauri Stars in the Small Magellanic Cloud
| dc.creator | Ivanov, Valentin D. | |
| dc.creator | Jayawardhana, Ray | |
| dc.date | 2002-05-29 | |
| dc.date.accessioned | 2026-07-25T18:39:12Z | |
| dc.description | The Small Magellanic Cloud (SMC) is an excellent laboratory to study the formation of solar-mass stars in a low-metallicity environment, similar to the conditions expected in the early phases of galactic evolution. Here we present preliminary results from a search for low-mass pre-main-sequence stars in the SMC based on Hubble Space Telescope archival data. Candidates are selected on the basis of their H_alpha emission and location in the [(F675W-F814W), F814W] color-magnitude diagram. We discuss characteristics of our candidate T Tauri sample and possible follow up work. | |
| dc.description | 5 pages, presented at the IAOC Workshop on "Galactic Star Formation Across the Stellar Mass Spectrum" held in La Serena, Chile, March 2002; to be published in the ASP Conference Series, edited by J. M. De Buizer | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0205496 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0205496 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/57294 | |
| dc.subject | Astrophysics | |
| dc.title | T Tauri Stars in the Small Magellanic Cloud | |
| dc.type | text |