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EASY SIGNED

Ejection Accretion Structures in YSOs (EASY)

Total Cost €

EC-Contrib. €

Partnership

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EASY project word cloud

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

shocks infrared origin campaigns clouds zone kinematics stellar interferometry stars spectrograph james see model mid young discriminating solar resolution approved abundant source mass space near ysos rays spatial variability yso observations observational disks astrophysical magellanic nirspec configuration miri competing jet larger cosmic mhd collimated au hydrodynamic agree ten for launched magnetic geometries few scales objects central strength outflows parent nature region diagnostics telescope instrument jwst initially magneto flow predict proximity give epoch mind engine discovering computational image jets acquiring link ideas webb radio energy nearest models ionized times metallicity atomic accretion opportunity outflow star protostars close

Project "EASY" data sheet

The following table provides information about the project.

Coordinator	DUBLIN INSTITUTE FOR ADVANCED STUDIES Organization address address: Burlington Road 10 city: DUBLIN postcode: 4 website: www.dias.ie 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	Ireland [IE]
Total cost	1˙853˙090 €
EC max contribution	1˙853˙090 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2016-ADG
Funding Scheme	ERC-ADG
Starting year	2017
Duration (year-month-day)	from 2017-10-01 to 2022-09-30

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	DUBLIN INSTITUTE FOR ADVANCED STUDIES DUBLIN INSTITUTE FOR ADVANCED STUDIES Organization address address: Burlington Road 10 city: DUBLIN postcode: 4 website: www.dias.ie contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	IE (DUBLIN)	coordinator	1˙853˙090.00

Map

Project objective

For a number of reasons, in particular their proximity and the abundant range of diagnostics to determine their characteristics, outflows from young stellar objects (YSOs) offer us the best opportunity of discovering how astrophysical jets are generated and the nature of the link between outflows and their accretion disks. Models predict that the jet is initially launched from within 0.1 to a few au of the star and focused on scales at most ten times larger. Thus, even for the nearest star formation region, we need high spatial resolution to image the “central engine” and test current models. With these ideas in mind, and the availability of a whole new set of observational and computational resources, it is proposed to investigate the origin of YSO jets, and the jet/accretion zone link, using a number of highly novel approaches to test magneto-hydrodynamic (MHD) models including: (a) Near-infrared interferometry to determine the spatial distribution and kinematics of the outflow as it is launched as a way of discriminating between competing models. (b) A multi-epoch study of the strength and configuration of the magnetic field of the parent star to see whether model values and geometries agree with observations and the nature of its variability. (c) Examining, through high spatial resolution radio observations, how the ionized component of these jets are collimated very close to the source and how shocks in the flow can give rise to low energy cosmic rays. (d) Use the James Webb Space Telescope (JWST) and, in particular, the Mid-Infrared Instrument (MIRI) and Near-Infrared Spectrograph (NIRSpec) to investigate with high spatial resolution atomic jets from protostars that are still acquiring most of their mass. In addition, we will study how accretion is affected by metallicity by studying young solar-like stars in the low metallicity Magellanic Clouds. In all cases the required observational campaigns have been approved.

Publications

List of publications.
year	authors and title	journal	last update
2019	A. Sanna, L. Moscadelli, C. Goddi, M. BeltrÃ¡n, C. L. Brogan, A. Caratti o Garatti, C. Carrasco-GonzÃ¡lez, T. R. Hunter, F. Massi, M. Padovani Protostellar Outflows at the EarliesT Stages (POETS) published pages: L3, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834551	Astronomy & Astrophysics 623	2019-06-06
2018	M. Koutoulaki, R. Garcia Lopez, A. Natta, A. Caratti o Garatti, D. Coffey, J. Sanchez-Bermudez, T. P. Ray The circumstellar environment of HDÂ 50138 revealed by VLTI/AMBER at high angular resolution published pages: A90, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201832814	Astronomy & Astrophysics 614	2019-06-06
2019	E. Koumpia, K. M. Ababakr, W. J. de Wit, R. D. Oudmaijer, A. Caratti o Garatti, P. Boley, H. Linz, S. Kraus, J. S. Vink, J.-B. Le Bouquin Resolving the MYSO binaries PDS 27 and PDS 37 with VLTI/PIONIER published pages: L5, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834624	Astronomy & Astrophysics 623	2019-06-06
2018	R. Fedriani, A. Caratti o Garatti, D. Coffey, R. Garcia Lopez, S. Kraus, G. Weigelt, B. Stecklum, T. P. Ray, C. M. Walmsley Parsec-scale jets driven by high-mass young stellar objects published pages: A126, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201732180	Astronomy & Astrophysics 616	2019-06-06
2018	G. D. C. Teixeira, M. S. N. Kumar, L. Smith, P. W. Lucas, C. Morris, J. Borissova, M. J. P. F. G. Monteiro, A. Caratti o Garatti, C. Contreras PeÃ±a, D. Froebrich, J. F. Gameiro Photometric variability of massive young stellar objects published pages: A41, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833667	Astronomy & Astrophysics 619	2019-06-06
2018	Paola Pinilla, Antonella Natta, Carlo F. Manara, Luca Ricci, Aleks Scholz, Leonardo Testi Resolved millimeter-dust continuum cavity around the very low mass young star CIDA 1 published pages: A95, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201832690	Astronomy & Astrophysics 615	2019-06-06
2018	Odysseas Dionatos, Tom Ray, Manuel GÃ¼del Herschel spectral-line mapping of the HH211 protostellar system published pages: A84, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833057	Astronomy & Astrophysics 616	2019-06-06
2018	S J D Purser, R E Ainsworth, T P Ray, D A Green, A M Taylor, A M M Scaife Constraining the nature of DG Tau Aâ€™s thermal and non-thermal radio emission published pages: 5532-5542, ISSN: 0035-8711, DOI: 10.1093/mnras/sty2649	Monthly Notices of the Royal Astronomical Society 481/4	2019-06-06
2018	R. Cesaroni, L. Moscadelli, R. Neri, A. Sanna, A. Caratti o Garatti, J. EislÃ¶ffel, B. Stecklum, T. Ray, C. M. Walmsley Radio outburst from a massive (proto)star published pages: A103, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201732238	Astronomy & Astrophysics 612	2019-06-06
2018	Garatti, Alessio Caratti o Supersize me! Jets from massive young stellar objects published pages: , ISSN: , DOI:	Star Formation Newsletter 1	2019-06-06
2019	M. Koutoulaki, S. Facchini, C. F. Manara, A. Natta, R. Garcia Lopez, R. Fedriani, A. Caratti o Garatti, D. Coffey, T. P. Ray Exploring the dimming event of RW Aurigae A through multi-epoch VLT/X-shooter spectroscopy published pages: A49, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834713	Astronomy & Astrophysics 625	2019-06-06

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