Add to ORKGNear infrared photometry at J, H, and K was obtained for 82 galaxies from the IRAS minisurvey. The near infrared colors of these galaxies cover a larger range in J-H and H-K than do normal field spiral galaxies, and evidence is presented of a tighter correlation between the near and far infrared emission in far infrared bright galaxies than exists between the far infrared and the visible emission. These results suggest the presence of dust in the far infrared bright galaxies, with hot dust emission contributing to the 2.2 micron emission, and extinction by dust affecting both the near infrared colors and the visible luminosities. In addition, there is some indication that the infrared emission in many of the minisurvey galaxies is coming fr...
Aperture photometry from our own observations and the literature is presented for the 12 μm galaxies...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
Pointed IRAS observations and ground based observations are used to determine the infrared propertie...
Near infrared photometry at J, H, and K was obtained for 82 galaxies from the IRAS minisurvey. The n...
Forty-seven galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR)⩾ 10^(11) L...
J, H, K, L', and N observations of galaxies detected at 12 microns by IRAS are combined with IRAS fl...
Results from a study of the far infrared properties of the brightest galaxies in the IRAS survey are...
A total of 86 galaxies have been detected at 60 μm in the high galactic latitude portion of the IRAS...
We use empirical techniques to interpret the near-infrared (near-IR) colours of a sample of 5800 gal...
These studies of the infrared colors of reflection nebulae, HL HI clouds, HII regions and external g...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
Several arguments can be made to study the continuum emission from dust in galaxies at wavelengths b...
A physical interpretation is proposed for the color-color diagram of galaxies which are powered only...
Very little surface photometry of normal galaxies has yet been performed in the near ...
Models for the infrared emission from Infrared Astronomy Satellite (IRAS) galaxies by Rowan-Robinson...
Aperture photometry from our own observations and the literature is presented for the 12 μm galaxies...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
Pointed IRAS observations and ground based observations are used to determine the infrared propertie...
Near infrared photometry at J, H, and K was obtained for 82 galaxies from the IRAS minisurvey. The n...
Forty-seven galaxies from the IRAS Bright Galaxy Sample with infrared luminosities L_(IR)⩾ 10^(11) L...
J, H, K, L', and N observations of galaxies detected at 12 microns by IRAS are combined with IRAS fl...
Results from a study of the far infrared properties of the brightest galaxies in the IRAS survey are...
A total of 86 galaxies have been detected at 60 μm in the high galactic latitude portion of the IRAS...
We use empirical techniques to interpret the near-infrared (near-IR) colours of a sample of 5800 gal...
These studies of the infrared colors of reflection nebulae, HL HI clouds, HII regions and external g...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
Several arguments can be made to study the continuum emission from dust in galaxies at wavelengths b...
A physical interpretation is proposed for the color-color diagram of galaxies which are powered only...
Very little surface photometry of normal galaxies has yet been performed in the near ...
Models for the infrared emission from Infrared Astronomy Satellite (IRAS) galaxies by Rowan-Robinson...
Aperture photometry from our own observations and the literature is presented for the 12 μm galaxies...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
Pointed IRAS observations and ground based observations are used to determine the infrared propertie...