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BEYONDCO SIGNED

Using fine structure line emission to observe the life-cycle of molecular clouds

Total Cost €

EC-Contrib. €

Partnership

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BEYONDCO project word cloud

Explore the words cloud of the BEYONDCO project. It provides you a very rough idea of what is the project "BEYONDCO" about.

feedback peak gas tools observational nature engines little monoxide simulations ci dissociated deeply density probe supply accessible tracers environments driving poor formed planetary evolution stellar compare star diffuse newly photons scenarios carbon forms genesis ultimately energetic herschel easily atomic regions numerical cii signatures temperature understand astrophysics mc destroyed dynamic ionised form dynamical setting interstellar structural oxygen stars assembled galactic radiation physical profile densest turbulence evolve local sofia timescale underpins alongside clouds myr co dense galaxies mcs oi fellow molecular destruction

Project "BEYONDCO" data sheet

The following table provides information about the project.

Coordinator	CARDIFF UNIVERSITY Organization address address: NEWPORT ROAD 30-36 city: CARDIFF postcode: CF24 ODE website: www.cardiff.ac.uk contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	United Kingdom [UK]
Total cost	183˙454 €
EC max contribution	183˙454 € (100%)
Programme	1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
Code Call	H2020-MSCA-IF-2015
Funding Scheme	MSCA-IF-EF-ST
Starting year	2016
Duration (year-month-day)	from 2016-10-06 to 2018-10-05

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	CARDIFF UNIVERSITY CARDIFF UNIVERSITY Organization address address: NEWPORT ROAD 30-36 city: CARDIFF postcode: CF24 ODE website: www.cardiff.ac.uk contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	UK (CARDIFF)	coordinator	183˙454.00

Map

Project objective

The formation of stars underpins all of astrophysics, from driving the evolution of galaxies to setting the conditions for the genesis of planetary systems. Stars form deeply embedded in the densest regions of molecular clouds (MCs), but we still know very little about how MCs are assembled and destroyed -- the two processes that ultimately set the timescale over which stars can form. Since carbon monoxide (CO) forms up to 10 Myr after the MC forms and is easily dissociated by energetic photons, it is a poor probe of MC formation and stellar feedback.

This project aims to determine the range of conditions under which MCs are formed and destroyed using newly accessible tracers of MCs and their environments: ionised carbon ([CII]), atomic carbon ([CI]) and atomic oxygen ([OI]). Together with CO, these tracers supply a comprehensive structural and dynamical profile of MC environments. In a sample of galactic clouds, we will measure the gas density, temperature and the local interstellar radiation field. We will compare observed dynamic signatures to simulations to MC formation scenarios, and we will determine the peak turbulence driving scale and the nature of stellar feedback in dense and diffuse gas.

This project makes timely use of new observational capabilities offered by Herschel and SOFIA alongside results of state-of-the-art numerical simulations. Using these tools together, the fellow will determine the physical processes driving the formation and destruction of MCs, which can be applied to better understand how galaxies evolve as star formation engines.

Publications

List of publications.
year	authors and title	journal	last update
2017	K. A. Marsh, A. P. Whitworth, O. Lomax, S. E. Ragan, U. Becciani, L. CambrÃ©sy, A. Di Giorgio, D. Eden, D. Elia, P. Kacsuk, S. Molinari, P. Palmeirim, S. Pezzuto, N. Schneider, E. Sciacca, F. Vitello Multitemperature mapping of dust structures throughout the Galactic Plane using the PPMAP tool with Herschel Hi-GAL data published pages: 2730-2742, ISSN: 0035-8711, DOI: 10.1093/mnras/stx1723	Monthly Notices of the Royal Astronomical Society 471/3	2019-04-18
2016	S. E. Ragan, T. J. T. Moore, D. J. Eden, M. G. Hoare, D. Elia, S. Molinari The prevalence of star formation as a function of Galactocentric radius published pages: 3123-3129, ISSN: 0035-8711, DOI: 10.1093/mnras/stw1870	Monthly Notices of the Royal Astronomical Society 462/3	2019-04-18
2018	S E Ragan, T J T Moore, D J Eden, M G Hoare, J S Urquhart, D Elia, S Molinari The role of spiral arms in Milky Way star formation published pages: 2361-2373, ISSN: 0035-8711, DOI: 10.1093/mnras/sty1672	Monthly Notices of the Royal Astronomical Society 479/2	2019-04-18
2018	M. R. Rugel, H. Beuther, S. Bihr, Y. Wang, J. Ott, A. Brunthaler, A. Walsh, S. C. O. Glover, P. F. Goldsmith, L. D. Anderson, N. Schneider, K. M. Menten, S. E. Ragan, J. S. Urquhart, R. S. Klessen, J. D. Soler, N. Roy, J. Kainulainen, T. Henning, F. Bigiel, R. J. Smith, F. Wyrowski, S. N. Longmore OH absorption in the first quadrant of the Milky Way as seen by THOR published pages: A159, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731872	Astronomy & Astrophysics 618	2019-04-18
2017	Sarah E Ragan The role of spiral arms in Milky Way star formation published pages: 565, ISSN: , DOI:	Memorie della Societa Astronomica Italiana 88	2019-04-18
2017	Davide Elia, S. Molinari, E. Schisano, M. Pestalozzi, S. Pezzuto, M. Merello, A. Noriega-Crespo, T. J. T. Moore, D. Russeil, J. C. Mottram, R. Paladini, F. Strafella, M. Benedettini, J. P. Bernard, A. Di Giorgio, D. J. Eden, Y. Fukui, R. Plume, J. Bally, P. G. Martin, S. E. Ragan, S. E. Jaffa, F. Motte, L. Olmi, N. Schneider, L. Testi, F. Wyrowski, A. Zavagno, L. Calzoletti, F. Faustini, P. Natoli, P. Palmeirim, F. Piacentini, L. Piazzo, G. L. Pilbratt, D. Polychroni, A. Baldeschi, M. T. BeltrÃ¡n, N. Billot, L. CambrÃ©sy, R. Cesaroni, P. GarcÃa-Lario, M. G. Hoare, M. Huang, G. Joncas, S. J. Liu, B. M. T. Maiolo, K. A. Marsh, Y. Maruccia, P. MÃ¨ge, N. Peretto, K. L. J. Rygl, P. Schilke, M. A. Thompson, A. Traficante, G. Umana, M. Veneziani, D. Ward-Thompson, A. P. Whitworth, H. Arab, M. Bandieramonte, U. Becciani, M. Brescia, C. Buemi, F. Bufano, R. Butora, S. Cavuoti, A. Costa, E. Fiorellino, A. Hajnal, T. Hayakawa, P. Kacsuk, P. Leto, G. Li Causi, N. Marchili, S. Martinavarro-Armengol, A. Mercurio, M. Molinaro, G. Riccio, H. Sano, E. Sciacca, K. Tachihara, K. Torii, C. Trigilio, F. Vitello, H. Yamamoto The Hi-GAL compact source catalogue â€“ I. The physical properties of the clumps in the inner Galaxy (âˆ’71$_{.}^{circ}$0 < â„“ < 67$_{.}^{circ}$0) published pages: 100-143, ISSN: 0035-8711, DOI: 10.1093/mnras/stx1357	Monthly Notices of the Royal Astronomical Society 471/1	2019-04-18
2018	Paul C. Clark, Simon C. O. Glover, Sarah E. Ragan, Ana Duarte-Cabral Tracing the formation of molecular clouds via [CII], [CI] and CO emission published pages: , ISSN: , DOI:		2019-04-18
2018	A T Barnes, J D Henshaw, P Caselli, I JimÃ©nez-Serra, J C Tan, F Fontani, A Pon, S Ragan Similar complex kinematics within two massive, filamentary infrared dark clouds published pages: 5268-5289, ISSN: 0035-8711, DOI: 10.1093/mnras/sty173	Monthly Notices of the Royal Astronomical Society 475/4	2019-04-18

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