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ABDES

An astrochemical study of the early evolutionary stages of sub-stellar mass objects

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EC-Contrib. €

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Partnership

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Project "ABDES" data sheet

The following table provides information about the project.

Coordinator
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV 

Organization address
address: HOFGARTENSTRASSE 8
city: Munich
postcode: 80539
website: www.mpg.de

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 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

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV DE (Munich) coordinator 159˙460.00

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 Project objective

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.

 Publications

year authors and title journal last update
List of publications.
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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