Diagnostics of dust obscured galactic nuclei with ISO spectroscopy
Soon after the IRAS mission, the first ever mission in exploring the Infrared world from space, it was realised that there exists a great number of galaxy populations that are extremely luminous at infrared wavelengths. Yet, their optical output was significantly smaller when compared to their infra...
Päätekijä: | Rigopoulou, D |
---|---|
Aineistotyyppi: | Conference item |
Julkaistu: |
1997
|
Samankaltaisia teoksia
-
CLOUD DISTRIBUTION IN OBSCURING TORI OF ACTIVE GALACTIC NUCLEI
Tekijä: E. Yu. Bannikova
Julkaistu: (2015-09-01) -
Obscured active galactic nuclei triggered in compact star-forming galaxies
Tekijä: Chang, Y, et al.
Julkaistu: (2016) -
ISO-SWS spectroscopy of Arp 220: A highly obscured starburst galaxy
Tekijä: Sturm, E, et al.
Julkaistu: (1996) -
A High Fraction of Heavily X-Ray-obscured Active Galactic Nuclei
Tekijä: Christopher M. Carroll, et al.
Julkaistu: (2023-01-01) -
X-ray Redshifts for Obscured Active Galactic Nuclei with AXIS Deep and Intermediate Surveys
Tekijä: Alessandro Peca, et al.
Julkaistu: (2024-06-01)