Name
9739
Title
Are We Missing the Dominant Sites of Star Formation in Local UV-Bright Starbursts?
URL
https://hst.esac.esa.int/ehst/#/pages/search;proposal=9739;TAPCLIENT=DOI
DOI
https://doi.org/10.5270/esa-9pbpi3v
Author
Chandar, Rupali
Description
This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9739&mission=hst
Publication
A Radio View of Star Formation in II Zw 40 High Resolution Radio and Optical Observations of the Central Starburst in the Low-metallicity Dwarf Galaxy II Zw 40 Integral field near-infrared spectroscopy of II Zw 40 On the Feedback from Super Stellar Clusters. I. The Structure of Giant H II Regions and H II Galaxies Physical Properties of II Zw 40s Super Star Cluster and Nebula: New Insights and Puzzles from UV Spectroscopy Properties of free-free, dust and CO emissions in the starbursts of blue compact dwarf galaxies Testing Models for Molecular Gas Formation in Galaxies: Hydrostatic Pressure or Gas and Dust Shielding? The Molecular Clouds Fueling A 1/5 Solar Metallicity Starburst The size-density relation of extragalactic H II regions
Instrument
ACS, ACS/HRC, NICMOS, NICMOS/NIC2, STIS/FUV-MAMA, STIS/NUV-MAMA
Temporal Coverage
2003-09-16T13:33:33Z/2004-07-12T07:46:55Z
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
2005-07-12T18:48:51Z
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, Chandar comma Rupali, 2005, 'Are We Missing the Dominant Sites of Star Formation in Local UV-Bright Starbursts?', 1.0, European Space Agency, https://doi.org/10.5270/esa-9pbpi3v Copy Example