Explore the words cloud of the PROMISE project. It provides you a very rough idea of what is the project "PROMISE" about.
The following table provides information about the project.
CHALMERS TEKNISKA HOEGSKOLA AB
|Coordinator Country||Sweden [SE]|
|Total cost||1˙266˙750 €|
|EC max contribution||1˙266˙750 € (100%)|
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
|Duration (year-month-day)||from 2016-02-01 to 2021-01-31|
Take a look of project's partnership.
|1||CHALMERS TEKNISKA HOEGSKOLA AB||SE (GOETEBORG)||coordinator||628˙987.00|
|2||MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV||DE (Munich)||participant||637˙762.00|
Understanding the physical processes that control the life-cycle of the interstellar medium (ISM) is one of the key themes in the astrophysics of galaxies today. This importance originates from the role of the ISM as the birthplace of new stars, and therefore, as an indivisible component of galaxy evolution. Exactly how the conversion of the ISM to stars takes place is intricately linked to how the internal structure of the cold, molecular clouds in the ISM forms and evolves. Despite this pivotal role, our picture of the molecular cloud structure has a fundamental lacking: it is based largely on observations of low-mass molecular clouds. Yet, it is the massive, giant molecular clouds (GMCs) in which most stars form and which impact the ISM of galaxies most. I present a program that will fill this gap and make profound progress in the field. We have developed a new observational technique that provides an unparalleled view of the structure of young GMCs. I also have developed a powerful tool to study the most important structural characteristics of molecular clouds, e.g., the probability distribution of volume densities, which have not been accessible before. With this program, the full potential of these tools will be put into use. We will produce a unique, high-fidelity column density data set for a statistically interesting volume in the Galaxy, including thousands of molecular clouds. The data set will be unmatched in its quality and extent, providing an unprecedented basis for statistical studies. We will then connect this outstanding observational view with state-of-the-art numerical simulations. This approach allows us to address the key question in the field: Which processes drive the structure formation in massive molecular clouds, and how do they do it? Most crucially, we will create a new, observationally constrained framework for the evolution of the molecular cloud structure over the entire mass range of molecular clouds and star formation in the ISM.
|year||authors and title||journal||last update|
A T Barnes, S N Longmore, A Avison, Y Contreras, A Ginsburg, J D Henshaw, J M Rathborne, D L Walker, J Alves, J Bally, C Battersby, M T BeltrÃ¡n, H Beuther, G Garay, L Gomez, J Jackson, J Kainulainen, J M D Kruijssen, X Lu, E A C Mills, J Ott, T Peters
Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds
published pages: 283-303, ISSN: 0035-8711, DOI: 10.1093/mnras/stz796
|Monthly Notices of the Royal Astronomical Society 486/1||2019-07-02|
A. Fuente, D. G. Navarro, P. Caselli, M. Gerin, C. Kramer, E. Roueff, T. Alonso-Albi, R. Bachiller, S. Cazaux, B. Commercon, R. Friesen, S. GarcÃa-Burillo, B. M. Giuliano, J. R. Goicoechea, P. Gratier, A. Hacar, I. JimÃ©nez-Serra, J. Kirk, V. Lattanzi, J. C. Loison, J. Malinen, N. Marcelino, R. MartÃn-DomÃ©nech, G. MuÃ±oz-Caro, J. Pineda, M. Tafalla, B. Tercero, D. Ward-Thompson, S. P. TreviÃ±o-
Gas phase Elemental abundances in Molecular cloudS (GEMS)
published pages: A105, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834654
|Astronomy & Astrophysics 624||2019-07-02|
M. Mattern, J. Kainulainen, M. Zhang, H. Beuther
Structure and fragmentation of a high line-mass filament: Nessie
published pages: A78, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731778
|Astronomy & Astrophysics 616||2019-05-29|
T. S. M. Rayner, M. J. Griffin, N. Schneider, F. Motte, V. KÃ¶nyves, P. AndrÃ©, J. Di Francesco, P. Didelon, K. Pattle, D. Ward-Thompson, L. D. Anderson, M. Benedettini, J.-P. Bernard, S. Bontemps, D. Elia, A. Fuente, M. Hennemann, T. Hill, J. Kirk, K. Marsh, A. Menâ€™shchikov, Q. Nguyen Luong, N. Peretto, S. Pezzuto, A. Rivera-Ingraham, A. Roy, K. Rygl, Ã. SÃ¡nchez-Monge, L. Spinoglio, J. TigÃ©, S. P. TreviÃ±o-Morales, G. J. White
Far-infrared observations of a massive cluster forming in the Monoceros R2 filament hub
published pages: A22, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201630039
|Astronomy & Astrophysics 607||2019-05-29|
M. Tahani, R. Plume, J. C. Brown, J. Kainulainen
Helical magnetic fields in molecular clouds?
published pages: A100, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201732219
|Astronomy & Astrophysics 614||2019-05-29|
J D Henshaw, A Ginsburg, T J Haworth, S N Longmore, J M D Kruijssen, E A C Mills, V Sokolov, D L Walker, A T Barnes, Y Contreras, J Bally, C Battersby, H Beuther, N Butterfield, J E Dale, T Henning, J M Jackson, J Kauffmann, T Pillai, S Ragan, M Riener, Q Zhang
â€˜The Brickâ€™ is not a brick : a comprehensive study of the structure and dynamics of the central molecular zone cloud G0.253+0.016
published pages: 2457-2485, ISSN: 0035-8711, DOI: 10.1093/mnras/stz471
|Monthly Notices of the Royal Astronomical Society 485/2||2019-04-18|
M. Zhang, J. Kainulainen, M. Mattern, M. Fang, Th. Henning
Star-forming content of the giant molecular filaments in the Milky Way
published pages: A52, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201732400
|Astronomy & Astrophysics 622||2019-04-18|
J. D. Soler, H. Beuther, M. Rugel, Y. Wang, P. C. Clark, S. C. O. Glover, P. F. Goldsmith, M. Heyer, L. D. Anderson, A. Goodman, Th. Henning, J. Kainulainen, R. S. Klessen, S. N. Longmore, N. M. McClure-Griffiths, K. M. Menten, J. C. Mottram, J. Ott, S. E. Ragan, R. J. Smith, J. S. Urquhart, F. Bigiel, P. Hennebelle, N. Roy, P. Schilke
Histogram of oriented gradients: a technique for the study of molecular cloud formation
published pages: A166, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834300
|Astronomy & Astrophysics 622||2019-04-18|
M. Mattern, J. Kauffmann, T. Csengeri, J. S. Urquhart, S. Leurini, F. Wyrowski, A. Giannetti, P. J. Barnes, H. Beuther, L. Bronfman, A. Duarte-Cabral, T. Henning, J. Kainulainen, K. M. Menten, E. Schisano, F. Schuller
SEDIGISM: the kinematics of ATLASGAL filaments
published pages: A166, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833406
|Astronomy & Astrophysics 619||2019-02-26|
M. Riener, C. M. Faesi, J. Forbrich, C. J. Lada
Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
published pages: A81, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201730738
|Astronomy & Astrophysics 612||2019-05-28|
J. Kainulainen, A. M. Stutz, T. Stanke, J. Abreu-Vicente, H. Beuther, T. Henning, K. G. Johnston, S. T. Megeath
Resolving the fragmentation of high line-mass filaments with ALMA: the integral shaped filament in Orion A
published pages: A141, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201628481
|Astronomy & Astrophysics 600||2019-05-28|
M. R. Rugel, H. Beuther, S. Bihr, Y. Wang, J. Ott, A. Brunthaler, A. Walsh, S. C. O. Glover, P. F. Goldsmith
OH absorption in the first quadrant of the Milky Way as seen by THOR
published pages: , ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731872
|Astronomy & Astrophysics 618||2019-05-28|
R.-A. Chira, J. Kainulainen, J. C. IbÃ¡Ã±ez-MejÃa, Th. Henning, M.-M. Mac Low
On the fragmentation of filaments in a molecular cloud simulation
published pages: A62, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731836
|Astronomy & Astrophysics 610||2019-05-28|
J. Kainulainen, C. Federrath
Relationship between turbulence energy and density variance in the solar neighbourhood molecular clouds
published pages: L3, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201731028
|Astronomy & Astrophysics 608||2019-05-28|
Are you the coordinator (or a participant) of this project? Plaese send me more information about the "PROMISE" project.
For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.
Send me an email (firstname.lastname@example.org) and I put them in your project's page as son as possible.
Thanks. And then put a link of this page into your project's website.
The information about "PROMISE" are provided by the European Opendata Portal: CORDIS opendata.