Case studies

Stefano Bovino; Tommaso Grassi; Jonathan Holdship; Inga Kamp; Alessandro Lupi; Christian Rab; Dominik Schleicher; Serena Viti

doi:10.1016/B978-0-32-391746-9.00024-9

Case studies

Stefano Bovino, Tommaso Grassi, Jonathan Holdship, Inga Kamp, Alessandro Lupi, Christian Rab, Dominik Schleicher, Serena Viti

Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Chapter › Academic › peer-review

Abstract

This chapter will discuss the main features and caveats related to some of the typical astrophysical problems. We will discuss applications of the chemistry at zero- and very-low-metallicity during high-redshift structure formation (first stars, galaxies, and SMBH), and in metal-polluted gas, together with the effects due to the presence of X-ray and UV radiation in the first galaxies. We will then examine the modeling of the star-forming regions, and the prestellar cores, focusing on the chemistry and the thermal processes. Finally, we will discuss the thermochemistry in the different parts of a protoplanetary disk.

Original language	English
Title of host publication	Astrochemical Modeling
Subtitle of host publication	Practical Aspects of Microphysics in Numerical Simulations
Editors	Stefano Bovino, Tommaso Grassi
Publisher	Springer
Chapter	14
Pages	365-398
Number of pages	34
ISBN (Electronic)	9780323917469
ISBN (Print)	9780323972574
DOIs	https://doi.org/10.1016/B978-0-32-391746-9.00024-9
Publication status	Published - 12-Jan-2024

Keywords

first galaxies
first stars
first supermassive black holes
Primordial chemistry
protoplanetary disks
protostars
star-forming regions

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10.1016/B978-0-32-391746-9.00024-9

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AU - Bovino, Stefano

AU - Grassi, Tommaso

AU - Holdship, Jonathan

AU - Kamp, Inga

AU - Lupi, Alessandro

AU - Rab, Christian

AU - Schleicher, Dominik

AU - Viti, Serena

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AB - This chapter will discuss the main features and caveats related to some of the typical astrophysical problems. We will discuss applications of the chemistry at zero- and very-low-metallicity during high-redshift structure formation (first stars, galaxies, and SMBH), and in metal-polluted gas, together with the effects due to the presence of X-ray and UV radiation in the first galaxies. We will then examine the modeling of the star-forming regions, and the prestellar cores, focusing on the chemistry and the thermal processes. Finally, we will discuss the thermochemistry in the different parts of a protoplanetary disk.

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KW - first stars

KW - first supermassive black holes

KW - Primordial chemistry

KW - protoplanetary disks

KW - protostars

KW - star-forming regions

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M3 - Chapter

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BT - Astrochemical Modeling

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A2 - Grassi, Tommaso

PB - Springer

ER -

Case studies

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