Name | 14140 |
Title | Using UV-bright Milky Way Halo Stars to Probe Star-Formation Driven Winds as a Function of Disk Scale Height |
URL | https://hst.esac.esa.int/ehst/#/pages/search;proposal=14140;TAPCLIENT=DOI |
DOI | https://doi.org/10.5270/esa-1ov5uf2 |
Author | Werk, Jessica Kay |
Description | This is a scientific proposal for HST mission. For specific information please visit https:\\archive.stsci.edu\proposal_search.php?id=14140&mission=hst |
Publication | Galactic Gas Flows from Halo to Disk: Tomography and Kinematics at the Milky Way’s Disk-Halo Interface, Bish, Hannah V.,Werk, Jessica K.,Prochaska, J. Xavier, The Astrophysical Journal, 882, 2019-09-01 00:00:00, 2019ApJ...882...76B||The Nature of Ionized Gas in the Milky Way Galactic Fountain, Werk, Jessica K.,Rubin, Kate H. R.,Bish, Hannah V., The Astrophysical Journal, 887, 2019-12-01 00:00:00, 2019ApJ...887...89W |
Instrument | COS/FUV |
Temporal Coverage | 2015-12-17T16:26:45Z/2016-06-25T12:18:04Z |
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 | 2017-06-25T13:00:50Z |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Werk, Jessica Kay, 2017, 14140, 1.0, European Space Agency, https://doi.org/10.5270/esa-1ov5uf2 |