A dataset provided by the European Space Agency

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 Ways Disk-Halo Interface
  • The Nature of Ionized Gas in the Milky Way Galactic Fountain
Instrument COS, 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
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, Werk comma Jessica Kay, 2017, 'Using UV-bright Milky Way Halo Stars to Probe Star-Formation Driven Winds as a Function of Disk Scale Height', 1.0, European Space Agency, https://doi.org/10.5270/esa-1ov5uf2