scholarly journals The Near‐ and Mid‐Infrared Continuum Emission of Seyfert Nuclei: Constraints on the Models of Obscuring Tori

1998 ◽  
Vol 496 (1) ◽  
pp. 117-132 ◽  
Author(s):  
Dario Fadda ◽  
Giuliano Giuricin ◽  
Gian Luigi Granato ◽  
Donatella Vecchies
Keyword(s):  
Continuum Emission ◽  
Mid Infrared ◽  
Infrared Continuum

scholarly journals The Extraordinary Outburst in the Massive Protostellar System NGC 6334 I-MM1: Strong Increase in Mid-Infrared Continuum Emission

2021 ◽  
Vol 912 (1) ◽  
pp. L17
Author(s):  
T. R. Hunter ◽  
C. L. Brogan ◽  
J. M. De Buizer ◽  
A. P. M. Towner ◽  
C. D. Dowell ◽  
...  
Keyword(s):  
Continuum Emission ◽  
Strong Increase ◽  
Mid Infrared ◽  
Ngc 6334 ◽  
Infrared Continuum

scholarly journals POLYCYCLIC AROMATIC HYDROCARBON AND MID-INFRARED CONTINUUM EMISSION IN Az> 4 SUBMILLIMETER GALAXY

2014 ◽  
Vol 786 (1) ◽  
pp. 31 ◽  
Author(s):  
Dominik A. Riechers ◽  
Alexandra Pope ◽  
Emanuele Daddi ◽  
Lee Armus ◽  
Christopher L. Carilli ◽  
...  
Keyword(s):  
Polycyclic Aromatic Hydrocarbon ◽  
Aromatic Hydrocarbon ◽  
Continuum Emission ◽  
Mid Infrared ◽  
Polycyclic Aromatic ◽  
Infrared Continuum

scholarly journals The relation between AGN hard X-ray emission and mid-infrared continuum from ISO spectra: Scatter and unification aspects

2004 ◽  
Vol 418 (2) ◽  
pp. 465-473 ◽  
Author(s):  
D. Lutz ◽  
R. Maiolino ◽  
H. W. W. Spoon ◽  
A. F. M. Moorwood
Keyword(s):  
Mid Infrared ◽  
X Ray ◽  
Infrared Continuum

scholarly journals Infrared Radiation from Evolved Stars

1990 ◽  
Vol 139 ◽  
pp. 118-120
Author(s):  
William K. Rose
Keyword(s):  
Milky Way ◽  
Background Radiation ◽  
Stellar Winds ◽  
Red Giants ◽  
Total Contribution ◽  
Mid Infrared ◽  
Evolved Stars ◽  
Infrared Measurements ◽  
Infrared Background ◽  
Infrared Continuum

OH/IR stars and carbon stars are examples of evolved stars known to lose mass rapidly. In a recent paper (Rose 1987) we have described calculations of infrared continuum radiation from dust in stellar winds from red giants. We compare calculated radiative models with recent infrared measurements and estimate the total contribution of evolved stars to the mid-infrared background radiation observed from the Milky Way and M31.

scholarly journals The mid-infrared spectral characteristics of blazars

2014 ◽  
Vol 10 (S313) ◽  
pp. 93-94
Author(s):  
Howard A. Smith ◽  
F. Massaro ◽  
R. D'Abrusco ◽  
A. Paggi ◽  
P. Cowperthwaite ◽  
...  
Keyword(s):  
Large Fraction ◽  
Spectral Characteristics ◽  
Continuum Emission ◽  
Spectral Features ◽  
Mid Infrared ◽  
Infrared Spectral ◽  
Infrared Spectrometer ◽  
Γ Ray ◽  
Followup Studies ◽  
The Continuum

AbstractWe previously reported discovering that blazars have distinctive infrared colors as seen in the WISE mission. Of particular note are γ-ray blazars, the locus of whose colors roughly overlaps with QSOs contours but which is more tightly delimited and bluer than ULIRGs and Seyferts. Since a large fraction of γ-ray sources are unassociated with any point source, but are expected to be blazars, identifying a WISE-candidate blazar in the γ-ray source field enables efficient followup studies. In an effort to better understand why blazars have these colors, we reduced and analyzed Spitzer Infrared Spectrometer (IRS) measurements on 73 blazars of varying types, some at several epochs. These spectra can be used to study the continuum emission (non-thermal), and search for atomic or other spectral features.

Mid‐infrared Continuum of Starburst Nuclei: Contribution from Hot Large Grains within HiiRegions?

1997 ◽  
Vol 484 (1) ◽  
pp. 222-229 ◽  
Author(s):  
Hideaki Mouri ◽  
Kimiaki Kawara ◽  
Yoshiaki Taniguchi
Keyword(s):  
Mid Infrared ◽  
Infrared Continuum
Sign in / Sign up

Export Citation Format

Share Document