Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy
Artikel i vetenskaplig tidskrift, 2024
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is affected by the nearby massive stars, and which portions of those GMCs eventually collapse into star forming regions. The complex interactions of those gas, dust and stellar populations form what has come to be known as the ecology of our Galaxy. Because we are deeply embedded in the plane of our Galaxy, it takes up a significant fraction of the sky, with complex dust lanes scattered throughout the optically recognizable bands of the Milky Way. These bands become bright at (sub-)millimetre wavelengths, where we can study dust thermal emission and the chemical and kinematic signatures of the gas. To properly study such large-scale environments, requires deep, large area surveys that are not possible with current facilities. Moreover, where stars form, so too do planetary systems, growing from the dust and gas in circumstellar discs, to planets and planetesimal belts. Understanding the evolution of these belts requires deep imaging capable of studying belts around young stellar objects to Kuiper belt analogues around the nearest stars. Here we present a plan for observing the Galactic Plane and circumstellar environments to quantify the physical structure, the magnetic fields, the dynamics, chemistry, star formation, and planetary system evolution of the galaxy in which we live with AtLAST; a concept for a new, 50m single-dish sub-mm telescope with a large field of view which is the only type of facility that will allow us to observe our Galaxy deeply and widely enough to make a leap forward in our understanding of our local ecology.
The Galaxy
Submillimeter Surveys
Astronomical instrumentation methods and techniques
Telescopes
Submillimeter planetary systems
solar neighborhood
Submillimeter ISM
Submillimeter Magnetic fields
Författare
Pamela Klaassen
Royal Observatory
A. Traficante
Istituto nazionale di astrofisica (INAF)
M. T. Beltrán
Osservatorio Astrofisico di Arcetri
Kate Pattle
University College London (UCL)
M. Booth
Royal Observatory
Joshua Lovell
Harvard-Smithsonian Center for Astrophysics
J. P. Marshall
Academia Sinica
A. Hacar
Universiteit Leiden
Universität Wien
Brandt Gaches
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Caroline Bot
Observatoire Astronomique de Strasbourg
Nicolas Peretto
Cardiff University
T. Stanke
Max-Planck-Gesellschaft
Doris Arzoumanian
National Astronomical Observatory of Japan
A. Duarte-Cabral
Cardiff University
G. Duchene
Université Grenoble Alpes
University of California
D. J. Eden
Armagh Observatory and Planetarium
Antonio Hales
National Radio Astronomy Observatory
J. K. F. Mann
Massachusetts Institute of Technology (MIT)
Patricia Luppe
Trinity College Dublin
Friedrich-Schiller-Universität Jena
Sebastian Marino
University of Exeter
Elena Redaelli
Max-Planck-Gesellschaft
Andrew Rigby
University of Leeds
A. Sanchez-Monge
Institut de Ciènces de l'Espai
E. Schisano
Istituto nazionale di astrofisica (INAF)
Dmitry Semenov
Max-Planck-Gesellschaft
S. Spezzano
Max-Planck-Gesellschaft
Mark Thompson
University of Leeds
F. Wyrowski
Max-Planck-Gesellschaft
C. Cicone
Universitetet i Oslo
Tony Mroczkowski
European Southern Observatory (ESO)
M. A. Cordiner
NASA Goddard Space Flight Center
Luca Di Mascolo
Universita degli Studi di Trieste
IFPU - Institute for Fundamental Physics of the Universe
Laboratoire Joseph-Louis Lagrange
Osservatorio Astronomico di Trieste
D. Johnstone
University of Victoria
National Research Council Canada
E. van Kampen
European Southern Observatory (ESO)
Minju Lee
Cosmic Dawn Center (DAWN)
Danmarks Tekniske Universitet (DTU)
Daizhong Liu
Chinese Academy of Sciences
Max-Planck-Gesellschaft
T. J. Maccarone
Texas Tech University at Lubbock
Amélie Saintonge
Max-Planck-Gesellschaft
University College London (UCL)
M. W.L. Smith
Cardiff University
Alexander Thelen
California Institute of Technology (Caltech)
S. Wedemeyer
Universitetet i Oslo
Open Research Europe
27325121 (eISSN)
Vol. 4 112Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.12688/openreseurope.17450.1