Role of Dust and Gas in the Evolution of Galaxies
A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Galaxies and Clusters".
Deadline for manuscript submissions: closed (1 April 2021) | Viewed by 359
Special Issue Editors
Interests: galaxy/quasar co-evolution; quasar feedback; star formation in quasar hosts; reddened quasars; multi-wavelength observations
Interests: imaging supermassive black holes; accretion physics of AGNs; gas kinematics and stellar dynamics; multifrequency SED modeling; sparse image processing
Special Issue Information
Dear Colleagues,
Studies into the role of dust and gas in the evolution of galaxies have received a major uplift with the advent of sensitive instruments and facilities such as the ALMA, Keck, and the VLT. To establish a major reference mark, we aim to explore the relationship between star formation, nuclear activity, and gas/dust in galaxies. We invite contributions to this Special Issue from the community that address the connection between the gas/dust and accreting supermassive black holes in quasar host galaxies, the nature of hot/cold molecular flows in quasars at different redshifts and across the electromagnetic spectrum, and the prospects of detecting first stars in galaxies in the timeframe of JWST.
Research on the panchromatic view of galaxies and their role in characterizing the cosmological ladder as proposed here fits neatly within the scope of the journal.
Dr. Clare Wethers
Dr. Venkatessh Ramakrishna
Guest Editors
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Keywords
- galaxy evolution
- nuclear feedback
- co-evolution
- dust obscuration
- star formation
- quasars
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