CO/H2 Abundance Ratio 10-4 in a Protoplanetary Disk
Probing Protoplanetary Disk Winds with C II Absorption
The 1600 A Emission Bump in Protoplanetary Disks: A Spectral Signature of H2O Dissociation
The Evolution of Inner Disk Gas in Transition Disks
UV Fluorescence Traces Gas and Lya Evolution in Protoplanetary Disks
X-ray to NIR emission from AA Tauri during the dim state. Occultation of the inner disk and gas-to-dust ratio of the absorber
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2013-02-05T03:11:33Z/2013-09-21T14:42:54Z
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, France comma Kevin, 2014, 'Project WHIPS {Warm H2 In Protoplanetary Systems}: Direct Measurement of Molecular Abundances in Circumstellar Disks', 1.0, European Space Agency, https://doi.org/10.5270/esa-4vt1sya