The Starburst-Driven Molecular Wind in NGC 253 and the Suppression of Star Formation

@inproceedings{Bolatto2013TheSM,
  title={The Starburst-Driven Molecular Wind in NGC 253 and the Suppression of Star Formation},
  author={Alberto D. Bolatto and Steven R. Warren and Adam K. Leroy and Fabian Walter and Sylvain Veilleux and Eve C. Ostriker and J{\"u}rgen Ott and Martin A. Zwaan and D. B. Fisher and Axel Weiss and Erik W. Rosolowsky and Jacqueline A. Hodge},
  year={2013}
}
The under-abundance of very massive galaxies in the universe is frequently attributed to the effect of galactic winds. Although ionized galactic winds are readily observable most of the expelled mass is likely in cooler atomic and molecular phases. Expanding molecular shells observed in starburst systems such as NGC 253 and M 82 may facilitate the entrainment of molecular gas in the wind. While shell properties are well constrained, determining the amount of outflowing gas emerging from such… 

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