Small grains and IRAS colors

Journal Article · Thu Sep 01 04:00:00 EDT 1988 · Astrophys. J.; (United States)

DOI:https://doi.org/10.1086/166658· OSTI ID:6684130

Boulanger, F; Beichman, C; Helou, G; Desert, F X; Perault, M

The paper studies how infrared colors of dust emission from the interstellar medium vary with the energy density of the radiation field on the basis of IRAS observation of the California Nebula. The data suggest that color variations result from a combinatin of equilibrium emission from large grains, and nonequilibrium emission from small grains, with destruction of the small grains emitting at 12 microns at high energy density; it is estimated that 80 percent of these small particles are destroyed for an energy density in ultraviolet photons larger than 50 times that of the average interstellar radiation field in the solar neighborhood. In a color-color diagram, I(v)(60 microns)/I(v)(100 microns) versus I(v)(12 microns)/I(v)(25 microns), the California Nebula measurements at various distances to the ionizing star Zeta Per follow a sequence similar to that of galaxies. This result shows that the position of a galaxy along this sequence is a measure of the intensity of the radiation field in the regions responsible for the infrared emission. 25 references.

• Research Organization: California Institute of Technology, Pasadena (USA); Ecole Normale Superieure, Paris (France); NASA, Goddard Space Flight Center, Greenbelt, MD (USA)
• OSTI ID: 6684130
• Journal Information: Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 332; ISSN ASJOA
• Country of Publication: United States
• Language: English

Related Subjects

640105* -- Astrophysics & Cosmology-- Galaxies
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COLOR
COSMIC DUST
DUSTS
ELECTROMAGNETIC RADIATION
FAR INFRARED RADIATION
INFRARED RADIATION
INTERSTELLAR GRAINS
INTERSTELLAR SPACE
OPTICAL PROPERTIES
ORGANOLEPTIC PROPERTIES
PARTICLES
PHYSICAL PROPERTIES
RADIATIONS
SPACE
VARIATIONS