A dataset provided by the European Space Agency

Name 3961
Title ELEMENTAL ABUNDANCES IN EARLY-TYPE STARS - CYCLE 2 OBSERVATIONS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=3961;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-yw5kkfe
Author Leckrone, David S.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=3961&mission=hst
Publication
  • A Goddard High Resolution Spectrograph Atlas of Echelle Observations of the HGMN Star chi LUPI
  • Atomic Data for the Re II UV 1 Multiplet and the Rhenium Abundance in the HgMn-type Star kh Lupi
  • Constraining the very heavy elemental abundance peak in the chemically peculiar star kh Lupi, with new atomic data for Os II and Ir II
  • Experimental Pd II Oscillator Strengths and the Palladium Abundance in the HgMn-Type Star chi LUPI
  • New Zr II oscillator strengths and the zirconium conflict in the HgMn star chi LUPI
  • Theoretical Oscillator Strengths for Sr II and Y III, with Application to Abundances in the HgMn-Type Star kh Lupi
  • Very High Resolution Ultraviolet Spectroscopy of a Chemically Peculiar Star: Results of the chi LUPI Pathfinder Project
Instrument HRS, HRS/2
Temporal Coverage 1993-02-01T19:19:00Z/1993-02-02T08:43:16Z
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 1994-02-02T15:26:35Z
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, Leckrone comma David S., 1994, 'ELEMENTAL ABUNDANCES IN EARLY-TYPE STARS - CYCLE 2 OBSERVATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-yw5kkfe