A dataset provided by the European Space Agency

Name 13734
Title Probing the extreme wind confinement of the most magnetic O star with COS spectroscopy
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=13734;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-ezay91s
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=13734&mission=hst
Publication Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star, David-Uraz, A.,Erba, C.,Petit, V., Monthly Notices of the Royal Astronomical Society, 483, 2019-02-01 00:00:00, 2019MNRAS.483.2814D||New observations of NGC 1624-2 reveal a complex magnetospheric structure and underlying surface magnetic geometry, David-Uraz, A.,Petit, VĂ©ronique,Shultz, M. E., Monthly Notices of the Royal Astronomical Society, 501, 2021-02-01 00:00:00, 2021MNRAS.501.2677D
Instrument COS/FUV, COS/NUV
Temporal Coverage 2015-02-17T06:08:59Z/2015-10-06T18:24:42Z
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 2016-10-07T02:18:15Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016, Probing The Extreme Wind Confinement Of The Most Magnetic O Star With Cos Spectroscopy, 1.0, European Space Agency, https://doi.org/10.5270/esa-ezay91s