Star Formation as Seen by Low Mass Stars
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České vysoké učení technické v Praze
Czech Technical University in Prague
Czech Technical University in Prague
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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.
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Acta Polytechnica. 2014, vol. 1, no. 1, p. 113-117.
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Except where otherwised noted, this item's license is described as Creative Commons Attribution 4.0 International License