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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21d.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34T/44TD9GB
Repositorysid.inpe.br/mtc-m21d/2021/06.21.13.27   (restricted access)
Last Update2021:06.21.13.27.54 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m21d/2021/06.21.13.27.54
Metadata Last Update2022:04.03.19.23.55 (UTC) administrator
DOI10.3389/fspas.2021.655450
ISSN2296-987X
Citation KeyMendozaDuRoCoTaPaNy:2021:InAsGa
TitleInterrelations Between Astrochemistry and Galactic Dynamics
Year2021
MonthMay
Access Date2024, May 09
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size3074 KiB
2. Context
Author1 Mendoza, Edgar
2 Duronea, Nicolas
3 Ronso, Daniele
4 Corazza, Lia Camargo
5 van der Tak, Floris
6 Paron, Sérgio
7 Nyman, Lars-Ake
Group1
2
3
4 AST-CEA-DIPGR-INPE-MCTI-GOV-BR
Affiliation1 Universidade Federal do Rio de Janeiro (UFRJ)
2 Instituto de Astrofísica de La Plata
3 Universidade de São Paulo (USP)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
5 SRON Netherlands Institute for Space Research
6 Universidad de Buenos Aires
7 European Southern Observatory
Author e-Mail Address1 emendoza@astro.ufrj.br
JournalFrontiers in Astronomy and Space Sciences
Volume8
Pagese655450
History (UTC)2021-06-21 13:30:12 :: simone -> administrator :: 2021
2022-04-03 19:23:55 :: administrator -> simone :: 2021
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
Keywordsastrochemistry
galaxies: general
ISM: molecules
methods: miscellaneous
history and philosophy of astronomy
AbstractThis 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.
AreaCEA
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4. Conditions of access and use
Languageen
Target Filemendoza_2021.pdf
User Groupsimone
Visibilityshown
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3F2NE4L
8JMKD3MGPCW/46KTFK8
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2021/06.04.03.40
6. Notes
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