Dynamical Masses of Young Stars in Multiple Systems
Measurement of T Tauri Binaries Using the Hubble Space Telescope Fine Guidance Sensors
Properties of the Closest Young Binaries. I. DF Taus Unequal Circumstellar Disk Evolution
Instrument
FGS
Temporal Coverage
1993-10-25T01:42:49Z/1993-10-25T14:56:57Z
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, Simon comma Michal, 1994, 'MASSES OF PRE-MAIN SEQUENCE BINARY STARS-PART 2', 1.0, European Space Agency, https://doi.org/10.57780/esa-5k44txw