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Hot massive stars in M33: HST UV spectroscopy and photometry

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 1997Publisher:AIPJournal:AIP Conference Proceedings
Authors: Luciana Bianchi;

doi: 10.1063/1.53788

Hot massive stars in M33: HST UV spectroscopy and photometry

Abstract

HST is used to study massive star populations in galaxies of the Local Group beyond the Magellanic Clouds (M31, M33, NGC6822). The purpose is to compare massive star parameters in parent galaxies with different metallicities and star formation histories. Some results for hot stars in M33 are described here.

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Powered by OpenAIRE graph
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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