Extreme Star Formation
arXiv:1009.1416 · doi:10.1007/978-1-4020-9457-6_9
Abstract
Extreme star formation includes star formation in starbursts and regions forming super star clusters. We survey the current problems in our understanding of the star formation process in starbursts and super star clusters - initial mass functions, cluster mass functions, star formation efficiencies, and radiative feedback into molecular clouds - that are critical to our understanding of the formation and survival of large star clusters, topics that will be the drivers of the observations of the next decade.
appeared in "Astrophysics in the Next Decade: JWST and Concurrent Facilities", Astrophysics and Space Science Proceedings, 2009, ed. H. A. Thronson, M. Stiavelli, and A. G. G. M. Tielens, proceedings of the conference, Astrophysics in the Next Decade, 24-27 September 2007, Tucson, AZ
References in corpus (29)
- The GALEX Ultraviolet Atlas of Nearby Galaxies
- Slow Star Formation in Dense Gas: Evidence and Implications
- Variations of the Mid-IR Aromatic Features Inside and Among Galaxies
- A census of the Wolf-Rayet content in Westerlund 1 from near-infrared imaging and spectroscopy
- Equilibrium Star Cluster Formation
- On the Rapid Collapse and Evolution of Molecular Clouds
- The Initial Mass Function of the Massive Star-forming Region NGC 3603 from Near-Infrared Adaptive Optics observations
- The influence of residual gas expulsion on the evolution of the Galactic globular cluster system and the origin of the Population II halo
- The secrets of the nearest starburst cluster: II. The present-day mass function in NGC 3603
- Super Star Cluster Velocity Dispersions and Virial Masses in the M82 Nuclear Starburst
- The Massive Star Content of NGC 3603
- Molecules in galaxies
- An alternative method to study star cluster disruption
- Formaldehyde Densitometry of Starburst Galaxies
- The shape of the initial cluster mass function: what it tells us about the local star formation efficiency
- CO(1-0), CO(2-1) and Neutral Gas in NGC 6946: Molecular Gas in a Late-Type, Gas Rich, Spiral Galaxy
- Medium resolution 2.3 micron spectroscopy of the massive Galactic open cluster Westerlund 1
- Nuclear Bar Catalyzed Star Formation: 13^CO, C18^O and Molecular Gas Properties in the Nucleus of Maffei 2
- Inflows and Outflows in the Dwarf Starburst Galaxy NGC 5253: High-Resolution HI Observations
- The pressure confined wind of the massive and compact superstar cluster M82-A1
- Subarcsecond-Resolution Radio Maps of Nearby Spiral Galaxies
- VLA H53alpha and H92alpha line observations of the central region of NGC 253
- Surface Brightness Profiles for a sample of LMC, SMC and Fornax galaxy Globular Clusters
- Dynamical evolution of the mass function and radial profile of the Galactic globular cluster system
- Detection of the H92alpha recombination line from the starbursts in the Circinus galaxy and NGC 1808
- The Stellar Initial Mass Function in 2007: A Year for Discovering Variations
- VLA H53alpha observations of the central region of the Super Star Cluster Galaxy NGC 5253
- The Extraordinary Infrared Spectrum of NGC 1222 (Mkn 603)
- Young massive star clusters: globular cluster progenitors?