A dataset provided by the European Space Agency

Name 4110
Title THE PHYSICS OF MASSIVE O-STARS IN DIFFERENT PARENT GALAXIES. THE MAGELLANIC CLOUDS - PART 2
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=4110;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-i96splr
Author Kudritzki, Rolf-Peter
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=4110&mission=hst
Publication
  • A CNO Dichotomy among O2 Giant Spectra in the Magellanic Clouds
  • A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC
  • Cold diffuse interstellar medium of Magellanic Clouds: II. Physical conditions from excitation of C I and H2
  • Constraints on the Ionization Balance of Hot-Star Winds from FUSE Observations of O Stars in the Large Magellanic Cloud
  • Global hot-star wind models for stars from Magellanic Clouds
  • HSTUV measurements of wind structure and velocities in Local Group OB stars
  • Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
  • Measuring the Ionization of O Star Winds
  • New Gapless COS G140L Mode Proposed for Background-limited Far-UV Observations
  • Quantitative UV spectroscopy of early O stars in the Magellanic Clouds. The determination of the stellar metallicities
  • Revised Stellar Temperatures for Magellanic Cloud O Supergiants from Far Ultraviolet Spectroscopic Explorer and Very Large Telescope UV-Visual Echelle Spectrograph Spectroscopy
  • The Physics of Massive OB Stars in Different Parent Galaxies. I. Ultraviolet and Optical Spectral Morphology in 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
  • Ultraviolet Line Spectra of Metal-poor Star-forming Galaxies
  • UV Spectroscopy of Metal-Poor Massive Stars in the Small Magellanic Cloud
Instrument FOS/BL
Temporal Coverage 1992-10-20T16:52:59Z/1993-10-27T20:45:38Z
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 1994-10-29T16:35:33Z
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, Kudritzki comma Rolf-Peter, 1994, 'THE PHYSICS OF MASSIVE O-STARS IN DIFFERENT PARENT GALAXIES. THE MAGELLANIC CLOUDS - PART 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-i96splr