A Far-ultraviolet Atlas of Low-resolution Hubble Space Telescope Spectra of T Tauri Stars
Analysis of HST Ultraviolet Spectra for T Tauri Stars: Estimating the Interstellar Extinction and the Contribution from an Accretion Shock to the Emission-Continuum Formation
Constraints on the ionizing flux emitted by T Tauri stars
Evolution of X-ray and Far-ultraviolet Disk-dispersing Radiation Fields
Far-Ultraviolet H2 Emission from Circumstellar Disks
Lyman-a Absorption from Heliotail ENAs
Mid-IR spectra of pre-main sequence Herbig stars: An explanation for the non-detections of water lines
Peculiarities of the UV Continuum Energy Distribution for T Tauri Stars
The Mass Accretion Rates of Intermediate-Mass T Tauri Stars
The Spatial Distribution of Fluorescent H2 Emission near T Tauri
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2000-02-07T02:56:29Z/2000-09-20T08:08:47Z
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 comma Nuria, 2006, 'Mass accretion rates for pre-main sequence intermediate mass stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-qpws150