Impact of Low-Energy Cosmic Rays on Star Formation
In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengths and theoretical modelling have shown that low-energy cosmic rays ( < 1 TeV ) play a fundamental role in shaping t...
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| Veröffentlicht in: | Space Sci.Rev 2020-03, Vol.216 (2), Article 29 |
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| creator | Padovani, Marco Ivlev, Alexei V. Galli, Daniele Offner, Stella S. R. Indriolo, Nick Rodgers-Lee, Donna Marcowith, Alexandre Girichidis, Philipp Bykov, Andrei M. Kruijssen, J. M. Diederik |
| description | In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengths and theoretical modelling have shown that low-energy cosmic rays (
<
1
TeV
) play a fundamental role in shaping the chemical richness of the interstellar medium, determining the dynamical evolution of molecular clouds. In this review we summarise in a coherent picture the main results obtained by observations and by theoretical models of propagation and generation of cosmic rays, from the smallest scales of protostars and circumstellar discs, to young stellar clusters, up to Galactic and extragalactic scales. We also discuss the new fields that will be explored in the near future thanks to new generation instruments, such as: CTA, for the
γ
-ray emission from high-mass protostars; SKA and precursors, for the synchrotron emission at different scales; and ELT/HIRES, JWST, and ARIEL, for the impact of cosmic rays on exoplanetary atmospheres and habitability. |
| doi_str_mv | 10.1007/s11214-020-00654-1 |
| format | Article |
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<
1
TeV
) play a fundamental role in shaping the chemical richness of the interstellar medium, determining the dynamical evolution of molecular clouds. In this review we summarise in a coherent picture the main results obtained by observations and by theoretical models of propagation and generation of cosmic rays, from the smallest scales of protostars and circumstellar discs, to young stellar clusters, up to Galactic and extragalactic scales. We also discuss the new fields that will be explored in the near future thanks to new generation instruments, such as: CTA, for the
γ
-ray emission from high-mass protostars; SKA and precursors, for the synchrotron emission at different scales; and ELT/HIRES, JWST, and ARIEL, for the impact of cosmic rays on exoplanetary atmospheres and habitability.</description><identifier>ISSN: 0038-6308</identifier><identifier>EISSN: 1572-9672</identifier><identifier>DOI: 10.1007/s11214-020-00654-1</identifier><language>eng</language><publisher>Dordrecht: Springer Netherlands</publisher><subject>Aerospace Technology and Astronautics ; Astrochemistry ; Astrophysics ; Astrophysics and Astroparticles ; Cosmic rays ; Emission ; Extrasolar planets ; Gamma emission ; Habitability ; Interstellar chemistry ; Interstellar matter ; Interstellar medium ; Molecular clouds ; Physics ; Physics and Astronomy ; Planetary atmospheres ; Planetology ; Protostars ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Star & galaxy formation ; Star clusters ; Star Formation ; Wavelengths</subject><ispartof>Space Sci.Rev, 2020-03, Vol.216 (2), Article 29</ispartof><rights>Springer Nature B.V. 2020</rights><rights>Space Science Reviews is a copyright of Springer, (2020). All Rights Reserved.</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c419t-91e78942f11cdff8d5f498a62cafedacfc577f7b8489c3a764fd82e9b9d28f1b3</citedby><cites>FETCH-LOGICAL-c419t-91e78942f11cdff8d5f498a62cafedacfc577f7b8489c3a764fd82e9b9d28f1b3</cites><orcidid>0000-0002-3971-0910</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11214-020-00654-1$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11214-020-00654-1$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,881,27901,27902,41464,42533,51294</link.rule.ids><backlink>$$Uhttps://hal.science/hal-02507599$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Padovani, Marco</creatorcontrib><creatorcontrib>Ivlev, Alexei V.</creatorcontrib><creatorcontrib>Galli, Daniele</creatorcontrib><creatorcontrib>Offner, Stella S. R.</creatorcontrib><creatorcontrib>Indriolo, Nick</creatorcontrib><creatorcontrib>Rodgers-Lee, Donna</creatorcontrib><creatorcontrib>Marcowith, Alexandre</creatorcontrib><creatorcontrib>Girichidis, Philipp</creatorcontrib><creatorcontrib>Bykov, Andrei M.</creatorcontrib><creatorcontrib>Kruijssen, J. M. Diederik</creatorcontrib><title>Impact of Low-Energy Cosmic Rays on Star Formation</title><title>Space Sci.Rev</title><addtitle>Space Sci Rev</addtitle><description>In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengths and theoretical modelling have shown that low-energy cosmic rays (
<
1
TeV
) play a fundamental role in shaping the chemical richness of the interstellar medium, determining the dynamical evolution of molecular clouds. In this review we summarise in a coherent picture the main results obtained by observations and by theoretical models of propagation and generation of cosmic rays, from the smallest scales of protostars and circumstellar discs, to young stellar clusters, up to Galactic and extragalactic scales. We also discuss the new fields that will be explored in the near future thanks to new generation instruments, such as: CTA, for the
γ
-ray emission from high-mass protostars; SKA and precursors, for the synchrotron emission at different scales; and ELT/HIRES, JWST, and ARIEL, for the impact of cosmic rays on exoplanetary atmospheres and habitability.</description><subject>Aerospace Technology and Astronautics</subject><subject>Astrochemistry</subject><subject>Astrophysics</subject><subject>Astrophysics and Astroparticles</subject><subject>Cosmic rays</subject><subject>Emission</subject><subject>Extrasolar planets</subject><subject>Gamma emission</subject><subject>Habitability</subject><subject>Interstellar chemistry</subject><subject>Interstellar matter</subject><subject>Interstellar medium</subject><subject>Molecular clouds</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Planetary atmospheres</subject><subject>Planetology</subject><subject>Protostars</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Star & galaxy formation</subject><subject>Star clusters</subject><subject>Star Formation</subject><subject>Wavelengths</subject><issn>0038-6308</issn><issn>1572-9672</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNp9kE1LAzEURYMoWKt_wNWAKxfRl2QySZaltLYwIPixDmkmqVPaSU2mSv-9M47oztWDy7mHx0XomsAdARD3iRBKcgwUMEDBc0xO0IhwQbEqBD1FIwAmccFAnqOLlDYAfU2MEF3u9sa2WfBZGT7xrHFxfcymIe1qmz2ZY8pCkz23JmbzEHemrUNzic682SZ39XPH6HU-e5kucPn4sJxOSmxzolqsiBNS5dQTYivvZcV9rqQpqDXeVcZ6y4XwYiVzqSwzosh9JalTK1VR6cmKjdHt4H0zW72P9c7Eow6m1otJqfsMKAfBlfogHXszsPsY3g8utXoTDrHp3tOUCV7wgjHVUXSgbAwpRed_tQR0P4geduzMoL931L2aDaXUwc3axT_1P60vkQNzZg</recordid><startdate>20200301</startdate><enddate>20200301</enddate><creator>Padovani, Marco</creator><creator>Ivlev, Alexei V.</creator><creator>Galli, Daniele</creator><creator>Offner, Stella S. 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R. ; Indriolo, Nick ; Rodgers-Lee, Donna ; Marcowith, Alexandre ; Girichidis, Philipp ; Bykov, Andrei M. ; Kruijssen, J. M. 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R.</au><au>Indriolo, Nick</au><au>Rodgers-Lee, Donna</au><au>Marcowith, Alexandre</au><au>Girichidis, Philipp</au><au>Bykov, Andrei M.</au><au>Kruijssen, J. M. Diederik</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Impact of Low-Energy Cosmic Rays on Star Formation</atitle><jtitle>Space Sci.Rev</jtitle><stitle>Space Sci Rev</stitle><date>2020-03-01</date><risdate>2020</risdate><volume>216</volume><issue>2</issue><artnum>29</artnum><issn>0038-6308</issn><eissn>1572-9672</eissn><abstract>In recent years, exciting developments have taken place in the identification of the role of cosmic rays in star-forming environments. Observations from radio to infrared wavelengths and theoretical modelling have shown that low-energy cosmic rays (
<
1
TeV
) play a fundamental role in shaping the chemical richness of the interstellar medium, determining the dynamical evolution of molecular clouds. In this review we summarise in a coherent picture the main results obtained by observations and by theoretical models of propagation and generation of cosmic rays, from the smallest scales of protostars and circumstellar discs, to young stellar clusters, up to Galactic and extragalactic scales. We also discuss the new fields that will be explored in the near future thanks to new generation instruments, such as: CTA, for the
γ
-ray emission from high-mass protostars; SKA and precursors, for the synchrotron emission at different scales; and ELT/HIRES, JWST, and ARIEL, for the impact of cosmic rays on exoplanetary atmospheres and habitability.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s11214-020-00654-1</doi><orcidid>https://orcid.org/0000-0002-3971-0910</orcidid></addata></record> |
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| subjects | Aerospace Technology and Astronautics Astrochemistry Astrophysics Astrophysics and Astroparticles Cosmic rays Emission Extrasolar planets Gamma emission Habitability Interstellar chemistry Interstellar matter Interstellar medium Molecular clouds Physics Physics and Astronomy Planetary atmospheres Planetology Protostars Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Star & galaxy formation Star clusters Star Formation Wavelengths |
| title | Impact of Low-Energy Cosmic Rays on Star Formation |
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