A dataset provided by the European Space Agency

Name 12799
Title The Unique Recurrent Nova T Pyxidis: The Transition to Quiescence
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=12799;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-zu27h20
Author Sion, Edward M.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=12799&mission=hst
Publication
  • Hubble Space Telescope Far Ultraviolet Spectroscopy of the Recurrent Nova T Pyxidis
  • The Long-term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis
  • The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst. III. The ultraviolet development from iron curtain through the post-X-ray turnoff
  • The spectroscopic evolution of the recurrent nova T Pyxidis during its 2011 outburst. II. The optically thin phase and the structure of the ejecta in recurrent novae
Instrument COS/FUV, COS/NUV, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2012-03-28T15:17:44Z/2012-03-28T19:16:31Z
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 2014-06-06T17:21:58Z
Last Update 2025-01-25
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Sion et al., 2014, 'The Unique Recurrent Nova T Pyxidis: The Transition to Quiescence', 1.0, European Space Agency, https://doi.org/10.5270/esa-zu27h20