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HIDDeN - Exploring the Hidden Dusty Nuclei of Galaxies

HIDDeN - Exploring the Hidden Dusty Nuclei of Galaxies

Objective

Luminous infrared galaxies (LIRGs) emit most of their bolometric luminosity in the far-infrared. They are mainly powered by extreme bursts of star formation and/or Active Galactic Nuclei (AGNs; accreting supermassive black holes (SMBHs)) in their centres. LIRGs are the closest examples of rapid evolution in galaxies and a detailed study of LIRGs is critical for our understanding of the cosmic evolution of galaxies and SMBHs. Centres of some LIRGs are deeply obscured and unreachable at optical, IR and even X-ray wavelengths. These hidden nuclei therefore represent a largely unexplored phase of the growth of central regions with their SMBHs. Large growth spurts are suspected to occur when the SMBHs are deeply embedded. Obscured AGNs thus can provide new constraints on the AGN duty cycle, give the full range of environments and astrophysical processes that drive the growth of SMBHs, and help to complete the picture of connections between the host galaxy and SMBH. Many dust embedded AGNs are still to be discovered as studies suggest that a significant fraction of SMBHs may be obscured in the local and more distant Universe.
In the HIDDeN project we use mm and submm observational methods to reach behind the curtain of dust in the most embedded centres of LIRGs, allowing us to undertake ground-breaking studies of heretofore hidden rapid evolutionary phases of nearby galaxy nuclei. HIDDeN takes advantage of emerging opportunities to address the nature of near-field, and redshift z=1-2, obscured AGNs/starbursts and their associated molecular inflows and outflows in the context of their evolution and the starburst-AGN connection. In particular we use the ALMA and NOEMA telescopes, supported by JVLA, LOFAR, HST and future JWST observations, to address four interconnected goals: A. Probing the Dusty Interiors of Compact Obscured Nuclei (CONs), B. The cold winds of change - Molecular Outflows from LIRGs and AGNs, C. The Co-Evolution of Starbursts and AGNs and D. Are there hidden CONs at z=1-2
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Host institution

CHALMERS TEKNISKA HOEGSKOLA AB

Address

-
41296 Goeteborg

Sweden

Activity type

Higher or Secondary Education Establishments

EU Contribution

€ 2 496 319

Beneficiaries (1)

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CHALMERS TEKNISKA HOEGSKOLA AB

Sweden

EU Contribution

€ 2 496 319

Project information

Grant agreement ID: 789410

Status

Ongoing project

  • Start date

    1 October 2018

  • End date

    30 September 2023

Funded under:

H2020-EU.1.1.

  • Overall budget:

    € 2 496 320

  • EU contribution

    € 2 496 319

Hosted by:

CHALMERS TEKNISKA HOEGSKOLA AB

Sweden