A dataset provided by the European Space Agency

Name 11625
Title Beyond the classical paradigm of stellar winds: Investigating clumping, rotation and the weak wind problem in SMC O stars
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11625;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-0kz3y5n
Author Hubeny, Ivan
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11625&mission=hst
Publication
  • Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
  • Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
  • Massive stars at low metallicity. Evolution and surface abundances of O dwarfs in the SMC
  • Massive stars in the Small Magellanic Cloud. Evolution, rotation, and surface abundances
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
  • Spectroscopic evolution of massive stars near the main sequence at low metallicity
  • Testing massive star evolution, star formation history, and feedback at low metallicity. Spectroscopic analysis of OB stars in the SMC Wing
Instrument COS, COS/FUV
Temporal Coverage 2009-11-01T01:05:41Z/2010-08-03T04:09:35Z
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 2011-08-03T15:06:08Z
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, Hubeny et al., 2011, 'Beyond the classical paradigm of stellar winds: Investigating clumping, rotation and the weak wind problem in SMC O stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-0kz3y5n