Star Formation as Seen by Low Mass Stars
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 - 4M<sub>ʘ</sub>), metallicities (0:1 - 1 Z<sub>ʘ</sub>) and ages (0:5 - 30 Myr). This is...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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CTU Central Library
2014-12-01
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| Series: | Acta Polytechnica CTU Proceedings |
| Online Access: | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2358 |
| _version_ | 1818061390863138816 |
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| author | Nino Panagia Guido De Marchi |
| author_facet | Nino Panagia Guido De Marchi |
| author_sort | Nino Panagia |
| collection | DOAJ |
| description | 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 - 4M<sub>ʘ</sub>), metallicities (0:1 - 1 Z<sub>ʘ</sub>) 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. |
| first_indexed | 2024-12-10T13:47:34Z |
| format | Article |
| id | doaj.art-e95662806400458bbf96c38df0243f16 |
| institution | Directory Open Access Journal |
| issn | 2336-5382 |
| language | English |
| last_indexed | 2024-12-10T13:47:34Z |
| publishDate | 2014-12-01 |
| publisher | CTU Central Library |
| record_format | Article |
| series | Acta Polytechnica CTU Proceedings |
| spelling | doaj.art-e95662806400458bbf96c38df0243f162022-12-22T01:46:20ZengCTU Central LibraryActa Polytechnica CTU Proceedings2336-53822014-12-011111311710.14311/APP.2014.01.01132170Star Formation as Seen by Low Mass StarsNino Panagia0Guido De Marchi1Supernova Ltd, OYV #131, Northsound Road, Virgin Gorda, British Virgin IslandsEuropean Space Agency, Keplerlaan 1, 2200 AG Noordwijk, NetherlandsUsing 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 - 4M<sub>ʘ</sub>), metallicities (0:1 - 1 Z<sub>ʘ</sub>) 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.https://ojs.cvut.cz/ojs/index.php/APP/article/view/2358 |
| spellingShingle | Nino Panagia Guido De Marchi Star Formation as Seen by Low Mass Stars Acta Polytechnica CTU Proceedings |
| title | Star Formation as Seen by Low Mass Stars |
| title_full | Star Formation as Seen by Low Mass Stars |
| title_fullStr | Star Formation as Seen by Low Mass Stars |
| title_full_unstemmed | Star Formation as Seen by Low Mass Stars |
| title_short | Star Formation as Seen by Low Mass Stars |
| title_sort | star formation as seen by low mass stars |
| url | https://ojs.cvut.cz/ojs/index.php/APP/article/view/2358 |
| work_keys_str_mv | AT ninopanagia starformationasseenbylowmassstars AT guidodemarchi starformationasseenbylowmassstars |