Chemical footprint of star formation feedback in M 82 on scales of similar to 100 pc

Ginard D.; Fuente A.; Garcia-Burillo S.Alonso-Albi T.Krips M.Gerin M.Neri R.Pilleri P.Usero A.Trevino-Morales S. P.

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Chemical footprint of star formation feedback in M 82 on scales of similar to 100 pc

机译：Chemical footprint of star formation feedback in M 82 on scales of similar to 100 pc

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Context. M 82 is one of the nearest and brightest starburst galaxies. It has been extensively studied in the past decade and by now is considered the prototypical extragalactic photon-dominated region (PDR) and a reference for studying star formation feedback.

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来源
《Astronomy and astrophysics》 |2015年第1期|共19页
作者
Ginard D.; Fuente A.; Garcia-Burillo S.Alonso-Albi T.Krips M.Gerin M.Neri R.Pilleri P.Usero A.Trevino-Morales S. P.;
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作者单位

OAN, IGN, Madrid 28800, Spain;

Observ Madrid, OAN, IGN, Madrid 28014, Spain;

Inst Radioastron Millimetr, St Martin Dheres 38406, FranceObserv Paris, CNRS, UMR 8112, LERMA, F-75231 Paris 05, FranceUniv Toulouse, UPS OMP, IRAP, F-31400 Toulouse, FranceInst Radioastron Milimetr IRAM Spain, Granada 18012, Spain;

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正文语种英语
中图分类天文学;
关键词
galaxies: individual: M82; galaxies: ISM; galaxies: starburst; ISM: abundances; ISM: molecules; astrochemistry;

Chemical footprint of star formation feedback in M 82 on scales of similar to 100 pc

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