Name | 13703 |
Title | The donor star winds in High-Mass X-ray Binaries |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=13703;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-ebijkc9 |
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=13703&mission=hst |
Publication | A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus {F}_{* }, f(H2), and Starlight Intensity, Jenkins, Edward B., The Astrophysical Journal, 872, 2019-02-01 00:00:00, 2019ApJ...872...55J||The stellar and wind parameters of six prototypical HMXBs and their evolutionary status, Hainich, R.,Oskinova, L. M.,Torrejón, J. M., Astronomy and Astrophysics, 634, 2020-02-01 00:00:00, 2020A&A...634A..49H |
Instrument | STIS/CCD, STIS/FUV-MAMA |
Temporal Coverage | 2015-01-01T11:41:33Z/2015-08-16T22:24:23Z |
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 | 2016-08-17T02:35:29Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2016, The Donor Star Winds In High-Mass X-Ray Binaries, 1.0, European Space Agency, https://doi.org/10.5270/esa-ebijkc9 |