A dataset provided by the European Space Agency

Name 11579
Title The Difference Between Neutral- and Ionized-Gas Metal Abundances in Local Star-Forming Galaxies with COS
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11579;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-8kuoex1
Author Aloisi, Alessandra
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11579&mission=hst
Publication
  • ALMA Observations toward the Starburst Dwarf Galaxy NGC 5253. I. Molecular Cloud Properties and Scaling Relations
  • Aperture and Resolution Effects on Ultraviolet Star-forming Properties: Insights from Local Galaxies and Implications for High-redshift Observations
  • Chemical enrichment and physical conditions in I Zw 18
  • CLusters in the Uv as EngineS (CLUES). II. Subkiloparsec-scale Outflows Driven by Stellar Feedback
  • CLusters in the UV as EngineS (CLUES). I. Survey Presentation and FUV Spectral Analysis of the Stellar Light
  • Constraining the Metallicities, Ages, Star Formation Histories, and Ionizing Continua of Extragalactic Massive Star Populations
  • First Cospatial Comparison of Stellar, Neutral-gas, and Ionized-gas Metallicities in a Metal-rich Galaxy: M83
  • Investigating Nearby Star-forming Galaxies in the Ultraviolet with HST/COS Spectroscopy. I. Spectral Analysis and Interstellar Abundance Determinations
  • Massive Star Formation in the Ultraviolet Observed with the Hubble Space Telescope
  • Metal-enriched galactic outflows shape the mass-metallicity relationship
  • Newly Improved Ionization Corrections for the Neutral Interstellar Medium: Enabling Accurate Abundance Determinations in Star-forming Galaxies throughout the Universe
  • Scaling Relations Between Warm Galactic Outflows and Their Host Galaxies
  • Shining a light on galactic outflows: photoionized outflows
  • Stars and gas in the most metal-poor galaxies - I. COS and MUSE observations of SBS 0335-052E
  • Synthetic Absorption Lines from Simulations of Multiphase Gas in Galactic Winds
  • Tackling the Saturation of Oxygen: The Use of Phosphorus and Sulfur as Proxies within the Neutral Interstellar Medium of Star-forming Galaxies
  • The Brightest Young Star Clusters in NGC 5253.
  • The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MegaSaura). II. Stacked Spectra
  • The mass and momentum outflow rates of photoionized galactic outflows
  • The Very Massive Star Content of the Nuclear Star Clusters in NGC 5253
Instrument ACS, ACS/SBC, COS, COS/FUV, COS/NUV
Temporal Coverage 2009-01-03T02:25:02Z/2011-05-04T15:16:00Z
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 2012-05-04T19:09:08Z
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, Aloisi comma Alessandra, 2012, 'The Difference Between Neutral- and Ionized-Gas Metal Abundances in Local Star-Forming Galaxies with COS', 1.0, European Space Agency, https://doi.org/10.5270/esa-8kuoex1