@Article{MendozaDuRoCoTaPaNy:2021:InAsGa,
author = "Mendoza, Edgar and Duronea, Nicolas and Ronso, Daniele and
Corazza, Lia Camargo and van der Tak, Floris and Paron,
S{\'e}rgio and Nyman, Lars-Ake",
affiliation = "{Universidade Federal do Rio de Janeiro (UFRJ)} and {Instituto de
Astrof{\'{\i}}sica de La Plata} and {Universidade de S{\~a}o
Paulo (USP)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {SRON Netherlands Institute for Space Research} and
{Universidad de Buenos Aires} and {European Southern
Observatory}",
title = "Interrelations Between Astrochemistry and Galactic Dynamics",
journal = "Frontiers in Astronomy and Space Sciences",
year = "2021",
volume = "8",
pages = "e655450",
month = "May",
keywords = "astrochemistry, galaxies: general, ISM: molecules, methods:
miscellaneous, history and philosophy of astronomy.",
abstract = "This paper presents a review of ideas that interconnect
astrochemistry and galactic dynamics. Since these two areas are
vast and not recent, each one has already been covered separately
by several reviews. After a general historical introduction, and a
needed quick review of processes such as stellar nucleosynthesis
that gives the base to understand the interstellar formation of
simple chemical compounds (e.g., H-2, GO, NH3, and H2O), we focus
on a number of topics that are at the crossing of the two big
areas, dynamics and astrochemistry. Astrochemistry is a
flourishing field that intends to study the presence and formation
of molecules as well as the influence of them on the structure,
evolution, and dynamics of astronomical objects. The progress in
the knowledge on the existence of new complex molecules and of
their process of formation originates from the observational,
experimental, and theoretical areas that compose the field. The
interfacing areas include star formation, protoplanetary disks,
the role of the spiral arms, and the chemical abundance gradients
in the galactic disk. It often happens that the physical
conditions in some regions of the interstellar medium are only
revealed by means of molecular observations. To organize a rough
classification of chemical evolution processes, we discuss about
how astrochemistry can act in three different contexts, namely,
the chemistry of the early universe, including external galaxies,
star-forming regions, and asymptotic giant branch (AGB) stars and
circumstellar envelopes. We mention that our research is
stimulated by plans for instruments and projects, such as the
ongoing Large Latin American Millimeter Array (LLAMA), which
consists in the construction of a 12 m sub-mm radio telescope in
the Andes. Thus, modern and new facilities can play a key role in
new discoveries not only in astrochemistry but also in radio
astronomy and related areas. Furthermore, the research on the
origin of life is also a stimulating perspective.",
doi = "10.3389/fspas.2021.655450",
url = "http://dx.doi.org/10.3389/fspas.2021.655450",
issn = "2296-987X",
language = "en",
targetfile = "mendoza_2021.pdf",
urlaccessdate = "19 maio 2024"
}