Name | 14177 |
Title | Identifying Ionization Mechanisms through Spatially-Resolved Neon Emission in the Jets of Sz 102 |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=14177;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-w7phdk5 |
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=14177&mission=hst |
Publication | Compositions of Planetary Debris around Dusty White Dwarfs, Xu, Siyi,Dufour, Patrick,Klein, Beth L., The Astronomical Journal, 158, 2019-12-01 00:00:00, 2019AJ....158..242X||Revealing Ionization Conditions of Sz 102 with Spatially Resolved [Ne III] Microjets, Liu, Chun-Fan,Shang, Hsien,Herczeg, Gregory J., The Astrophysical Journal, 909, 2021-03-01 00:00:00, 2021ApJ...909..196L |
Instrument | STIS/CCD |
Temporal Coverage | 2016-05-06T12:41:05Z/2016-05-06T15:04:29Z |
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 | 2017-05-06T17:51:21Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, 2017, Identifying Ionization Mechanisms Through Spatially-Resolved Neon Emission In The Jets Of Sz 102, 1.0, European Space Agency, https://doi.org/10.5270/esa-w7phdk5 |