de
Dario Colombo
© D. Colombo
Dr. Dario Colombo

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Zugehörigkeiten
  • Argelander Institut für Astronomie
  • Mathematisch-Naturwissenschaftliche Fakultät
Forschungsschwerpunkte
  • Interstellar medium
  • Milky Way structure
  • Star formation quenching
  • Galaxy evolution
My research focuses on understanding the interstellar medium (atomic, molecular and dust) and how its properties influence star formation and galaxy evolution. To this aim, I make use of data from large surveys of the Milky Way (such as SEDIGISM, OGHReS, and Hi-GAL) and nearby galaxies (such as PHANGS and EDGE-CALIFA), and sophisticated, machine learning-based algorithms (e.g. SCIMES).
Ausgewählte Publikationen

Colombo, D., Sanchez, S. F., Bolatto, A. D., Kalinova, V.,
Weiß, A., Wong, T., . . . Blitz, L. (2020, December). The
EDGE-CALIFA survey: exploring the role of molecular gas
on galaxy star formation quenching. A&A, 644, A97. doi:
10.1051/0004-6361/ 202039005

Colombo, D., Rosolowsky, E., Ginsburg, A., Duarte-Cabral,
A., & Hughes, A. (2015, December). Graph-based
interpretation of the molecular interstellar medium
segmen- tation. MNRAS, 454(2), 2067-2091. doi: 10.1093/
mnras/stv2063

Colombo, D., Hughes, A., Schinnerer, E., Meidt, S. E.,
Leroy, A. K., Pety, J., ... Kramer, C. (2014, March). The
PdBI Arcsecond Whirlpool Survey (PAWS): Envi-
ronmental Dependence of Giant Molecular Cloud
Properties in M51. ApJ, 784(1), 3. doi:
10.1088/0004-637X/784/1/3

Dario Colombo
© D. Colombo
Dr. Dario Colombo

Webseite

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