Accretion Rates for T Tauri Stars Using Nearly Simultaneous Ultraviolet and Optical Spectra
A Far-ultraviolet Atlas of Low-resolution Hubble Space Telescope Spectra of T Tauri Stars
Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks
Peculiarities of the UV Continuum Energy Distribution for T Tauri Stars
The Effects of UV Continuum and Lya Radiation on the Chemical Equilibrium of T Tauri Disks
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2002-01-12T12:46:48Z/2002-07-13T19:07:30Z
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, Calvet et al., 2003, 'Accretion in the planet-forming disks of the TW Hya association', 1.0, European Space Agency, https://doi.org/10.5270/esa-r4dp1h8