A dataset provided by the European Space Agency

Name 12211
Title Are Weak-Line T Tauri Stars Still Accreting?
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12211;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-96b0l7o
Author European Space Agency
Description This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=12211&mission=hst
Publication Short Gas Dissipation Timescales: Diskless Stars in Taurus and Chamaeleon I, Ingleby, Laura,Calvet, Nuria,Herczeg, Gregory, The Astrophysical Journal, 752, 2012-06-01 00:00:00, 2012ApJ...752L..20I
Instrument ACS, ACS/SBC
Temporal Coverage 2011-07-22T21:58:35Z/2012-02-18T12:51:08Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2013-02-18T19:25:08Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013, Are Weak-Line T Tauri Stars Still Accreting?, 1.0, European Space Agency, https://doi.org/10.5270/esa-96b0l7o