Star Formation as Seen by Low Mass Stars
dc.contributor.author | Panagia, Nino | |
dc.contributor.author | De Marchi, Guido | |
dc.date.accessioned | 2023-01-18T14:10:37Z | |
dc.date.available | 2023-01-18T14:10:37Z | |
dc.date.issued | 2014 | |
dc.identifier.citation | Acta Polytechnica. 2014, vol. 1, no. 1, p. 113-117. | |
dc.identifier.issn | 1210-2709 (print) | |
dc.identifier.issn | 1805-2363 (online) | |
dc.identifier.uri | http://hdl.handle.net/10467/105700 | |
dc.description.abstract | Using the Hubble Space Telescope (HST) we have characterised and compared the physical properties of a large sample of pre-main sequence (PMS) stars spanning a wide range of masses (0:5 - 4Mʘ), metallicities (0:1 - 1 Zʘ) and ages (0:5 - 30 Myr). This is presently the largest and most homogeneous sample of PMS objects with known physical properties. The main results of this ongoing study are briefly summarised here. | en |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | České vysoké učení technické v Praze | cs |
dc.publisher | Czech Technical University in Prague | en |
dc.relation.ispartofseries | Acta Polytechnica | |
dc.relation.uri | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2358 | |
dc.rights | Creative Commons Attribution 4.0 International License | en |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
dc.title | Star Formation as Seen by Low Mass Stars | |
dc.type | article | en |
dc.date.updated | 2023-01-18T14:10:37Z | |
dc.identifier.doi | 10.14311/APP.2014.01.0113 | |
dc.rights.access | openAccess | |
dc.type.status | Peer-reviewed | |
dc.type.version | publishedVersion |
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