Publication

The evolution of the atomic and molecular interstellar medium in star-forming galaxies

Popping, G., 2014, [S.l.]: [S.n.]. 197 p.

Research output: ThesisThesis fully internal (DIV)Academic

APA

Popping, G. (2014). The evolution of the atomic and molecular interstellar medium in star-forming galaxies. [S.l.]: [S.n.].

Author

Popping, Gergö. / The evolution of the atomic and molecular interstellar medium in star-forming galaxies. [S.l.] : [S.n.], 2014. 197 p.

Harvard

Popping, G 2014, 'The evolution of the atomic and molecular interstellar medium in star-forming galaxies', Doctor of Philosophy, University of Groningen, [S.l.].

Standard

The evolution of the atomic and molecular interstellar medium in star-forming galaxies. / Popping, Gergö.

[S.l.] : [S.n.], 2014. 197 p.

Research output: ThesisThesis fully internal (DIV)Academic

Vancouver

Popping G. The evolution of the atomic and molecular interstellar medium in star-forming galaxies. [S.l.]: [S.n.], 2014. 197 p.


BibTeX

@phdthesis{2b4dacd74da2454bbd77e35ff73e67c6,
title = "The evolution of the atomic and molecular interstellar medium in star-forming galaxies",
abstract = "In this thesis I developed models to make predictions for the atomic and molecular gas content of galaxies. Main results of my thesis include that the atomic hydrogen content of galaxies remained relatively constant with over the last 10 Billion years, whereas the molecular hydrogen content decreased by more than an order of magnitude during the same cosmic epoch. I furhermore found that the decline in the cosmic star-formation rate of our Universe is driven by a decrease in the gas content of galaxies, and by a decrease in the fraction of gas in galaxies that is eligible for star-formation. I also developed models that make predictions for the emission of atoms and molecules such as carbon, oxide, and carbonmonoxide. The results presented in this thesis will be extremely useful for future surveys with the newest generation of radio and sub-mm telescopes such as ALMA in Chile and the SKA in South-Afrika and Australia.",
author = "Gerg{\"o} Popping",
year = "2014",
language = "English",
isbn = "978-94-6259-352-7",
publisher = "[S.n.]",
school = "University of Groningen",

}

RIS

TY - THES

T1 - The evolution of the atomic and molecular interstellar medium in star-forming galaxies

AU - Popping, Gergö

PY - 2014

Y1 - 2014

N2 - In this thesis I developed models to make predictions for the atomic and molecular gas content of galaxies. Main results of my thesis include that the atomic hydrogen content of galaxies remained relatively constant with over the last 10 Billion years, whereas the molecular hydrogen content decreased by more than an order of magnitude during the same cosmic epoch. I furhermore found that the decline in the cosmic star-formation rate of our Universe is driven by a decrease in the gas content of galaxies, and by a decrease in the fraction of gas in galaxies that is eligible for star-formation. I also developed models that make predictions for the emission of atoms and molecules such as carbon, oxide, and carbonmonoxide. The results presented in this thesis will be extremely useful for future surveys with the newest generation of radio and sub-mm telescopes such as ALMA in Chile and the SKA in South-Afrika and Australia.

AB - In this thesis I developed models to make predictions for the atomic and molecular gas content of galaxies. Main results of my thesis include that the atomic hydrogen content of galaxies remained relatively constant with over the last 10 Billion years, whereas the molecular hydrogen content decreased by more than an order of magnitude during the same cosmic epoch. I furhermore found that the decline in the cosmic star-formation rate of our Universe is driven by a decrease in the gas content of galaxies, and by a decrease in the fraction of gas in galaxies that is eligible for star-formation. I also developed models that make predictions for the emission of atoms and molecules such as carbon, oxide, and carbonmonoxide. The results presented in this thesis will be extremely useful for future surveys with the newest generation of radio and sub-mm telescopes such as ALMA in Chile and the SKA in South-Afrika and Australia.

M3 - Thesis fully internal (DIV)

SN - 978-94-6259-352-7

PB - [S.n.]

CY - [S.l.]

ER -

ID: 14255706