Explore the words cloud of the ABDES project. It provides you a very rough idea of what is the project "ABDES" about.
The following table provides information about the project.
Coordinator |
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
Organization address contact info |
Coordinator Country | Germany [DE] |
Project website | http://www.mpe.mpg.de/6729630/news20170516 |
Total cost | 159˙460 € |
EC max contribution | 159˙460 € (100%) |
Programme |
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility) |
Code Call | H2020-MSCA-IF-2014 |
Funding Scheme | MSCA-IF-EF-ST |
Starting year | 2015 |
Duration (year-month-day) | from 2015-09-01 to 2017-08-31 |
Take a look of project's partnership.
# | ||||
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1 | MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV | DE (Munich) | coordinator | 159˙460.00 |
Astrochemistry is an inter-disciplinary field that provides an insight into the complex physical and chemical processes at play during the early evolutionary stages in star-formation. Over the last decade, while astrochemical studies have been conducted to understand the early evolutionary stages in high- and low-mass stars, similar work is essentially missing for the least massive stars, called brown dwarfs (BDs). BDs are ‘sub-stellar’ objects with insufficient mass to burn hydrogen in their cores and shine like stars, but are found as abundantly as Sun-like stars in star-forming regions, making them an equally vital constituent of our Galaxy. ABDES is an innovative inter-disciplinary project, which will deliver radically new advancements in our understanding of the astrochemical processes that occur during the early evolutionary stages in BD-formation. The objectives of ABDES are to characterize the physical and chemical structure of early-stage BDs, and study the fundamental role played by the accretion and outflow processes in shaping their evolution. With the advent of high-class telescopes and instruments with unparalleled sensitivities, it is now feasible to probe deep into the early evolutionary stages of BDs. To achieve these objectives, I have built the largest sample to date of early-stage BDs, using a new set of deep, high-sensitivity, multi-wavelength observations. ABDES will combine these observations with chemical/physical modelling techniques, and provide the first measurements on the astrochemical properties of early-stage BDs. Being an inter-disciplinary research division, the Centre for Astrochemical Studies at MPE, under the supervision of Prof. Caselli, is a great fit to this project, and provides excellent expertise and infrastructure for its successful implementation. ABDES is a pioneering study that will highlight the origins of the faintest stars in our Galaxy, and complete our understanding of star-formation toward the lowest mass end.
year | authors and title | journal | last update |
---|---|---|---|
2015 |
B. Riaz, E. T. Whelan HH 1158: THE LOWEST LUMINOSITY EXTERNALLY IRRADIATED HERBIG–HARO JET published pages: L31, ISSN: 2041-8213, DOI: 10.1088/2041-8205/815/2/L31 |
The Astrophysical Journal 815/2 | 2019-06-18 |
2017 |
B. Riaz, C. Briceño, E. T. Whelan, S. Heathcote First Large-scale Herbig–Haro Jet Driven by a Proto-brown Dwarf published pages: 47, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aa70e8 |
The Astrophysical Journal 844/1 | 2019-06-18 |
2016 |
B. Riaz, E. Vorobyov, D. Harsono, P. Caselli, K. Tikare, O. Gonzalez-Martin A MULTIWAVELENGTH CHARACTERIZATION OF PROTO-BROWN-DWARF CANDIDATES IN SERPENS published pages: 189, ISSN: 1538-4357, DOI: 10.3847/0004-637X/831/2/189 |
The Astrophysical Journal 831/2 | 2019-06-18 |
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The information about "ABDES" are provided by the European Opendata Portal: CORDIS opendata.
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