Publikationsdatum:
2019-06-28
Beschreibung:
Far-infrared fine-structuze lines of compact H II regions can provide reliable abundances throughout the Galactic plane. We present here our most recent results, which once analyzed, will help to constrain models of the abundance gradient in our galaxy.
Schlagwort(e):
ASTROPHYSICS
Materialart:
Astronomical Society of the Pacific, Airborne Astronomy Symposium on the Galactic Ecosystem: From Gas to Stars to Dust, Volume 73; p 111-114
Format:
text