Abstract
Using the Hubble Space Telescope, we have undertaken a systematic study 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). We have used WFPC2, ACS and WFC3 observations in the broad V an I bands and H˛ narrow filter to identify and characterise a large sample of PMS stars in star forming.
Cite
CITATION STYLE
APA
Beccari, G., de Marchi, G., Panagia, N., Romaniello, M., Sabbi, E., & Spezzi, L. (2014). An HST study of star formation in star-burst clusters. In Astrophysics and Space Science Proceedings (Vol. 36, pp. 481–483). Kluwer Academic Publishers. https://doi.org/10.1007/978-3-319-03041-8_96
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.
Already have an account? Sign in
Sign up for free