University of Hertfordshire

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Physical Processes in Star Formation

Research output: Contribution to journalArticlepeer-review

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Physical Processes in Star Formation. / Girichidis, Philipp; Offner, Stella S. R.; Kritsuk, Alexei G.; Klessen, Ralf S.; Hennebelle, Patrick; Kruijssen, J. M. Diederik; Krause, Martin G. H.; Glover, Simon C. O.; Padovani, Marco.

In: Space Science Reviews, Vol. 216, 68, 02.06.2020.

Research output: Contribution to journalArticlepeer-review

Harvard

Girichidis, P, Offner, SSR, Kritsuk, AG, Klessen, RS, Hennebelle, P, Kruijssen, JMD, Krause, MGH, Glover, SCO & Padovani, M 2020, 'Physical Processes in Star Formation', Space Science Reviews, vol. 216, 68. https://doi.org/10.1007/s11214-020-00693-8

APA

Girichidis, P., Offner, S. S. R., Kritsuk, A. G., Klessen, R. S., Hennebelle, P., Kruijssen, J. M. D., Krause, M. G. H., Glover, S. C. O., & Padovani, M. (2020). Physical Processes in Star Formation. Space Science Reviews, 216, [68]. https://doi.org/10.1007/s11214-020-00693-8

Vancouver

Girichidis P, Offner SSR, Kritsuk AG, Klessen RS, Hennebelle P, Kruijssen JMD et al. Physical Processes in Star Formation. Space Science Reviews. 2020 Jun 2;216. 68. https://doi.org/10.1007/s11214-020-00693-8

Author

Girichidis, Philipp ; Offner, Stella S. R. ; Kritsuk, Alexei G. ; Klessen, Ralf S. ; Hennebelle, Patrick ; Kruijssen, J. M. Diederik ; Krause, Martin G. H. ; Glover, Simon C. O. ; Padovani, Marco. / Physical Processes in Star Formation. In: Space Science Reviews. 2020 ; Vol. 216.

Bibtex

@article{5a8d7e2f15314e898ed0028b7087e5dd,
title = "Physical Processes in Star Formation",
abstract = " Star formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronomy from local star forming regions in the Milky Way up to high-redshift galaxies. From a theoretical perspective, star formation and feedback processes (radiation, winds, and supernovae) play a pivotal role in advancing our understanding of the physical processes at work, both individually and of their interactions. In this review we will give an overview of the main processes that are important for the understanding of star formation. We start with an observationally motivated view on star formation from a global perspective and outline the general paradigm of the life-cycle of molecular clouds, in which star formation is the key process to close the cycle. After that we focus on the thermal and chemical aspects in star forming regions, discuss turbulence and magnetic fields as well as gravitational forces. Finally, we review the most important stellar feedback mechanisms. ",
keywords = "astro-ph.GA, astro-ph.SR",
author = "Philipp Girichidis and Offner, {Stella S. R.} and Kritsuk, {Alexei G.} and Klessen, {Ralf S.} and Patrick Hennebelle and Kruijssen, {J. M. Diederik} and Krause, {Martin G. H.} and Glover, {Simon C. O.} and Marco Padovani",
note = "{\textcopyright} 2020 Springer-Verlag. The final publication is available at Springer via https://doi.org/10.1007/s11214-020-00693-8. ",
year = "2020",
month = jun,
day = "2",
doi = "10.1007/s11214-020-00693-8",
language = "English",
volume = "216",
journal = "Space Science Reviews",
issn = "0038-6308",
publisher = "Springer Netherlands",

}

RIS

TY - JOUR

T1 - Physical Processes in Star Formation

AU - Girichidis, Philipp

AU - Offner, Stella S. R.

AU - Kritsuk, Alexei G.

AU - Klessen, Ralf S.

AU - Hennebelle, Patrick

AU - Kruijssen, J. M. Diederik

AU - Krause, Martin G. H.

AU - Glover, Simon C. O.

AU - Padovani, Marco

N1 - © 2020 Springer-Verlag. The final publication is available at Springer via https://doi.org/10.1007/s11214-020-00693-8.

PY - 2020/6/2

Y1 - 2020/6/2

N2 - Star formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronomy from local star forming regions in the Milky Way up to high-redshift galaxies. From a theoretical perspective, star formation and feedback processes (radiation, winds, and supernovae) play a pivotal role in advancing our understanding of the physical processes at work, both individually and of their interactions. In this review we will give an overview of the main processes that are important for the understanding of star formation. We start with an observationally motivated view on star formation from a global perspective and outline the general paradigm of the life-cycle of molecular clouds, in which star formation is the key process to close the cycle. After that we focus on the thermal and chemical aspects in star forming regions, discuss turbulence and magnetic fields as well as gravitational forces. Finally, we review the most important stellar feedback mechanisms.

AB - Star formation is a complex multi-scale phenomenon that is of significant importance for astrophysics in general. Stars and star formation are key pillars in observational astronomy from local star forming regions in the Milky Way up to high-redshift galaxies. From a theoretical perspective, star formation and feedback processes (radiation, winds, and supernovae) play a pivotal role in advancing our understanding of the physical processes at work, both individually and of their interactions. In this review we will give an overview of the main processes that are important for the understanding of star formation. We start with an observationally motivated view on star formation from a global perspective and outline the general paradigm of the life-cycle of molecular clouds, in which star formation is the key process to close the cycle. After that we focus on the thermal and chemical aspects in star forming regions, discuss turbulence and magnetic fields as well as gravitational forces. Finally, we review the most important stellar feedback mechanisms.

KW - astro-ph.GA

KW - astro-ph.SR

U2 - 10.1007/s11214-020-00693-8

DO - 10.1007/s11214-020-00693-8

M3 - Article

VL - 216

JO - Space Science Reviews

JF - Space Science Reviews

SN - 0038-6308

M1 - 68

ER -