Year: 2014
Type: article
Abstract: Context. Images of spatially resolved astrophysical objects contain a wealth of morphological and dynamical information, and effectively extracting this information is of paramount importance for understanding the physics and evolution of these objects. The algorithms and methods currently employed for this purpose (such as Gaussian model fitting) often use simplified approaches to describe the structure of resolved objects.
Source: Astronomy and Astrophysics
Authors: Florent Mertens, Andrei Lobanov
Institutions: Max Planck Institute for Radio Astronomy, Universität Hamburg
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2170249695