Add to ORKGA physical interpretation is proposed for the color-color diagram of galaxies which are powered only by star formation. The colors of each galaxy result from the combination of two components: cirrus-like emission from the neutral disk, and warmer emission from regions directly involved in on-going star formation. This approach to modelling the emission is based on dust properties, but independent evidence for it is found in the relation between the color sequence and the luminosity sequence. Implications of data and interpretations are discussed and possible tests mentioned for the model
Connecting the observed rest-ultraviolet (UV) luminosities of high-z galaxies to their intrinsic lum...
Near infrared photometry at J, H, and K was obtained for 82 galaxies from the IRAS minisurvey. The n...
The ways in which recent infrared observations, particularly by the Infrared Astronomy Satellite (IR...
Models for the infrared emission from Infrared Astronomy Satellite (IRAS) galaxies by Rowan-Robinson...
16 pages, 11 figures, 2 tables. Appearing in the GALEX special issue of ApJ Supp. (29 papers)The col...
International audienceWe present a simple, largely empirical but physically motivated model to inter...
We use empirical techniques to interpret the near-infrared (near-IR) colours of a sample of 5800 gal...
We present a self-consistent model of the spectral energy distributions (SEDs) of spiral g...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
After the IRAS discovery of galaxies with large far-infrared to blue luminosity ratio, it has been p...
The UVJ color-color diagram is a popular and efficient method to distinguish between quiescent and s...
Context. Infrared (IR), sub-millimetre (sub-mm), and millimetre (mm) databases contain a huge quanti...
Unbiased analysis shows that IRAS data reliably differentiate between the early and late stages of s...
J, H, K, L', and N observations of galaxies detected at 12 microns by IRAS are combined with IRAS fl...
Connecting the observed rest-ultraviolet (UV) luminosities of high-z galaxies to their intrinsic lum...
Near infrared photometry at J, H, and K was obtained for 82 galaxies from the IRAS minisurvey. The n...
The ways in which recent infrared observations, particularly by the Infrared Astronomy Satellite (IR...
Models for the infrared emission from Infrared Astronomy Satellite (IRAS) galaxies by Rowan-Robinson...
16 pages, 11 figures, 2 tables. Appearing in the GALEX special issue of ApJ Supp. (29 papers)The col...
International audienceWe present a simple, largely empirical but physically motivated model to inter...
We use empirical techniques to interpret the near-infrared (near-IR) colours of a sample of 5800 gal...
We present a self-consistent model of the spectral energy distributions (SEDs) of spiral g...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
We have measured the near-infrared colors and the fluxes of individual pixels in 68 galaxies common ...
After the IRAS discovery of galaxies with large far-infrared to blue luminosity ratio, it has been p...
The UVJ color-color diagram is a popular and efficient method to distinguish between quiescent and s...
Context. Infrared (IR), sub-millimetre (sub-mm), and millimetre (mm) databases contain a huge quanti...
Unbiased analysis shows that IRAS data reliably differentiate between the early and late stages of s...
J, H, K, L', and N observations of galaxies detected at 12 microns by IRAS are combined with IRAS fl...
Connecting the observed rest-ultraviolet (UV) luminosities of high-z galaxies to their intrinsic lum...
Near infrared photometry at J, H, and K was obtained for 82 galaxies from the IRAS minisurvey. The n...
The ways in which recent infrared observations, particularly by the Infrared Astronomy Satellite (IR...