Name
15629
Title
MAssivE STaR Outflows (MAESTRO)
URL
https://hst.esac.esa.int/ehst/#/pages/search;proposal=15629;TAPCLIENT=DOI
DOI
https://doi.org/10.5270/esa-9vch8jq
Author
Mahy, Laurent
Description
This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=15629&mission=hst
Publication
Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2 Mapping the core of the Tarantula Nebula with VLT-MUSE - III. A template for metal-poor starburst regions in the visual and far-ultraviolet Optically thick structure in early B-type supergiant stellar winds at low metallicities Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
Instrument
COS, COS/FUV, COS/NUV, STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2019-11-14T14:31:33Z/2020-06-24T06:43:23Z
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
2020-12-24T10:53:56Z
Last Update
2025-01-25
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, Mahy et al., 2020, 'MAssivE STaR Outflows (MAESTRO)', 1.0, European Space Agency, https://doi.org/10.5270/esa-9vch8jq Copy Example