AK Sco, First Detection of a Highly Disturbed Atmosphere in a Pre-Main-Sequence Close Binary
Consistent dust and gas models for protoplanetary disks. IV. A panchromatic view of protoplanetary disks
Evidence for an Ionized Rotating Structure Around RW Aur
Evidence of Stellar-driven Outflows from the Classical T Tauri Star RY Tau
Hubble Space Telescope STIS Spectrum of RW Aurigae A: Evidence for an Ionized Beltlike Structure and Mass Ejection in Timescales of a Few Hours
Mid-IR spectra of pre-main sequence Herbig stars: An explanation for the non-detections of water lines
On the source of dense outflows from T Tauri stars - III. Winds driven from the star-disc shear layer
The X-Ray Properties of Moderate-Redshift Galaxy Groups Selected by Association with Gravitational Lenses
Wind/jet Formation in T Tauri Stars: Theory versus UV Observations
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
2000-09-16T13:48:42Z/2001-04-08T07:05:08Z
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, Gomez de Castro comma Ana Ines, 2001, 'High Density {~ 10^9 cm^-3} gas in the jet formation region of T Tauri stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-vts9wux
