Kenza Posted November 7, 2013 Share Posted November 7, 2013 The term H II refers to regions of interstellar dust abundant in Hydrogen which have been ionized by UV radiation from nearby hot stars and have had their electrons stripped off. Also, the roman numeral next to the element refers to the number of electrons that an atom is missing, in this case two electrons. How can a Hydrogen atom lose 2 electrons??? What am I missing here? Link to comment Share on other sites More sharing options...
JulianO Posted November 7, 2013 Share Posted November 7, 2013 Its confusing terminology - but its what we're stuck with. In astronomy you haveH2 - so called molecular hydrogen - what we see on Earth normally.H I - which is called atomic hydrogen - there is enough radiation to split the two atoms apart, but not enough to ionise it in the main.H II - is ionised hydrogen - stripped of it's electron, needing sufficient energy to kick the electrons away.Confusing - certainly, always annoyed me, but its what everyone uses in the field. Link to comment Share on other sites More sharing options...
Kenza Posted November 7, 2013 Author Share Posted November 7, 2013 I get it now! That is confusing. So basically the rule doesn't apply for Hydrogen as it does for other ionized atoms like S II or O III. Link to comment Share on other sites More sharing options...
JulianO Posted November 7, 2013 Share Posted November 7, 2013 No - its similar for O as well. Link to comment Share on other sites More sharing options...
cosmiquery Posted November 22, 2013 Share Posted November 22, 2013 Basically you subtract one from the roman numeral and that give you the number of missing electrons. Link to comment Share on other sites More sharing options...
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