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
Constraints to the magnetospheric properties of T Tauri stars - II. The Mg II ultraviolet feature
Constraints to the magnetospheric properties of T Tauri stars - I. The C II, Fe II and Si II ultraviolet features
CoolCAT
Estimating the Interstellar Extinction and the Contribution from an Accretion Shock to the Formation of Emission Continuum in DS Tau and DG Tau
Hot Gas Lines in T Tauri Stars
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
Mid-IR spectra of pre-main sequence Herbig stars: An explanation for the non-detections of water lines
Molecular hydrogen fluorescence and accretion in far-ultraviolet spectra of classical T Tauri stars
Probing Protoplanetary Disk Winds with C II Absorption
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
2000-08-24T18:41:06Z/2000-12-06T19:58:33Z
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., 2001, 'The Structure of the Accretion Flow on pre-main-sequence stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-xlzny4q
