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.
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
|Coordinator Country||Germany [DE]|
|Total cost||159˙460 €|
|EC max contribution||159˙460 € (100%)|
1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
|Duration (year-month-day)||from 2015-09-01 to 2017-08-31|
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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|
B. Riaz, E. T. Whelan
HH 1158: THE LOWEST LUMINOSITY EXTERNALLY IRRADIATED HERBIGâ€“HARO JET
published pages: L31, ISSN: 2041-8213, DOI: 10.1088/2041-8205/815/2/L31
|The Astrophysical Journal 815/2||2019-06-18|
B. Riaz, C. BriceÃ±o, E. T. Whelan, S. Heathcote
First Large-scale Herbigâ€“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|
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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