A dataset provided by the European Space Agency

Name 9412
Title The Physical Parameters of the Hottest, Most Luminous Stars as a Function of Metallicity
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9412;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-nel8roh
Author Massey, Philip Louis
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9412&mission=hst
Publication
  • A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds
  • 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
  • Nitrogen line spectroscopy in O-stars. III. The earliest O-stars
  • Optically thick structure in early B-type supergiant stellar winds at low metallicities
  • The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. I. A Sample of 20 Stars in the Magellanic Clouds
  • The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. II. Analysis of 20 More Magellanic Cloud Stars and Results from the Complete Sample
  • The Physical Properties and Effective Temperature Scale of O-Type Stars as a Function of Metallicity. III. More Results From the Magellanic Clouds
  • The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He II l1640 in young star clusters
  • The VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence
  • The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution
  • The Wolf-Rayet stars in the Large Magellanic Cloud. A comprehensive analysis of the WN class
Instrument STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage 2002-05-30T21:55:17Z/2003-08-05T17:35:56Z
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 2007-01-23T00:06:25Z
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, Massey et al., 2007, 'The Physical Parameters of the Hottest, Most Luminous Stars as a Function of Metallicity', 1.0, European Space Agency, https://doi.org/10.5270/esa-nel8roh