Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. VI. The Case of LH 95 in the Large Magellanic Cloud, Biazzo, K.,Beccari, Giacomo,De Marchi, Guido, The Astrophysical Journal, 875, 2019-04-01 00:00:00, 2019ApJ...875...51B||Pre-main sequence stars in LH 91, Carini, Roberta,Biazzo, K.,De Marchi, Guido, Astronomy and Astrophysics, 663, 2022-07-01 00:00:00, 2022A&A...663A..74C
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2013-05-26T18:46:32Z/2013-05-30T03:06:03Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, 2014, Characterizing The Mass Accretion Rates In Young Low-Mass Stars At Low Metallicity, 1.0, European Space Agency, https://doi.org/10.5270/esa-o10aq65