Hola,
¿eres nuevo aquí?

Regístrate gratis y conecta tu empresa con financiación pública, partners y proyectos.

Tengo cuenta

Regístrate

Ver video

PARSECDUST

Financiado

Cerrado

Supermassive black holes under the microscope Revealing the dusty environment o...

Supermassive black holes under the microscope Revealing the dusty environment of AGN on parsec scales with IR and sub mm interferometry The evolution of galaxies and their central supermassive black holes are intimately related. As such, it is of great interest to understand the active growth phase of these black holes and their influence on the surrounding host g... ver más

29/02/2016

SOUTHAMPTON

231K€

Presupuesto del proyecto: 231K€

Líder del proyecto

UNIVERSITY OF SOUTHAMPTON No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Fecha límite participación Sin fecha límite de participación.

Ver 2 Participantes

Financiación concedida El organismo FP7 notifico la concesión del proyecto el día 2016-02-29 No tenemos la información de la convocatoria

0% 100%

Información adicional privada

No hay información privada compartida para este proyecto. Habla con el coordinador.

2 Participantes

SOUTHAMPTON

0.00€ | Lider

UCPH

N.D. | Participante

Conecta tu I+D

¿Tienes un proyecto y buscas un partner? Gracias a nuestro motor inteligente podemos recomendarte los mejores socios y ponerte en contacto con ellos. Te lo explicamos en este video

Proyectos interesantes

DustOrigin The origin of cosmic dust in galaxies 2M€ Cerrado

DUST-IN-THE-WIND Dust in the wind a new paradigm for inflow and outflow str... 1M€ Cerrado

DUSTDEVILS The Dust Devils in Galaxy Centres 183K€ Cerrado

AYA2015-64346-C2-1-P LAS GALAXIAS CERCANAS Y LEJANAS Y SUS NUCLEOS ACTIVOS 121K€ Cerrado

EUR2021-122010 EN BUSCA DE UNA VISION OBSERVACIONAL COMPLETA DE LOS VIENTOS... 100K€ Cerrado

AGNPROBES Active Galactic Nuclei as probes of galaxy evolution 275K€ Cerrado

Líder del proyecto

UNIVERSITY OF SOUTHAMPTON No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 231K€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto The evolution of galaxies and their central supermassive black holes are intimately related. As such, it is of great interest to understand the active growth phase of these black holes and their influence on the surrounding host galaxies. I propose a project to study the outer, dusty region of mass accretion onto supermassive black holes with the objective to address the following open questions: * How is the accreting mass distributed? Do we see any dependence on the accretion state of the supermassive black holes? * Do we see a dusty wind that regulates or limits accretion on parsec scales? How does it work? Does this wind cause feedback reactions on the surrounding galaxy? * Why do dust emission features around supermassive black holes appear different than in the interstellar medium? Does the hard radiation from the black-hole environment change the dust composition? Each of these three topical units will be investigated in separate sub-projects that combine aspects of theory, modeling, and observations. More specifically I combine the latest high-angular resolution IR and sub-mm data from the frontline facilities VLTI and ALMA with models of the dust emission and of dynamical processes. As a main goal of this application I want to transfer my expertise in interferometry to Denmark to stimulate the use of ALMA and VLTI. These observatories are of prime interest to the European astronomical community as outlined in the ASTRONET framework and infrastructure documents. Via student training, teaching, and talks, I want to increase the appeal of this technique and its usage in Denmark, with new instruments about to be commissioned.

Conecta tu I+D

Entra hoy

¿Olvidé mi contraseña?

Financiación

Empresas

CTIs/Universidades

Proyectos

Investigadores