05.07.2013 Views

Peter BIERMANN (.pdf)

Peter BIERMANN (.pdf)

Peter BIERMANN (.pdf)

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Absorption line forest, excited by cosmic rays<br />

• These stars make magnetic fields, explode, and then<br />

make cosmic rays:<br />

• These cosmic rays excite characteristic transitions in<br />

massive gaseous shells of molecular surrounding the<br />

HNR<br />

• Absorption line forest: H2, H + 2 , H+ 3<br />

• Identify groups of lines, originating from specific HNRs,<br />

and in the beam-adding need to be able to identify each<br />

HNR separately<br />

20<br />

• In any beam of a telescope many such lines, so very<br />

high signal to noise required<br />

• If such lines confirmed, key signature for a) cosmic rays,<br />

and by inference b) magnetic fields - and all at a known<br />

redshift: line equivalent width − > mass scale

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!