A Candidate Protoplanet in the Taurus Star-forming Region
A near-infrared variability campaign of TMR-1: New light on the nature of the candidate protoplanet TMR-1C
JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region
Large-amplitude photometric variability of the candidate protoplanet TMR-1C
Multiple protostellar systems. II. A high resolution near-infrared imaging survey in nearby star-forming regions
Near-infrared imaging polarimetry of young stellar objects in r Ophiuchi
PROSAC: a submillimeter array survey of low-mass protostars. II. The mass evolution of envelopes, disks, and stars from the Class 0 through I stages
The circumstellar environment of the YSO TMR-1 and a revisit to the candidate very low-mass object TMR-1C
The Circumstellar Structure of the Class I Protostar TMC-1 (IRAS 04381+2540) from Hubble Space Telescope NICMOS Data
The Evolution of Circumstellar Disks in Ophiuchus Binaries
Instrument
NICMOS, NICMOS/NIC2
Temporal Coverage
1997-07-03T00:57:14Z/1997-12-20T10:15:04Z
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, Terebey comma Susan, 1998, 'The Small Scale Structure of Protostellar Disks and Infall Envelopes', 1.0, European Space Agency, https://doi.org/10.5270/esa-sl4or4j
