Work

Brightness temperature constraints from interferometric visibilities

Year: 2014

Type: article

Abstract: Context. The brightness temperature is an effective parameter that describes the physical properties of emitting material in astrophysical objects. It is commonly determined by imaging and modeling the structure of the emitting region and estimating its flux density and angular size.

Source: Astronomy and Astrophysics

DOI: 10.1051/0004-6361/201425084

Author: Andrei Lobanov

Institutions: Universität Hamburg, Max Planck Institute for Radio Astronomy

Language: English

Topic: Radio Astronomy Observations and Technology

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

Funders: National Science Foundation, National Radio Astronomy Observatory, Associated Universities

OpenAlex ID: W1983414154