Interstellar dust absorption features in the infrared spectrum of HH 100-IR: Searching for the nitrogen component of the ICES
We present observations of solid-state absorption features due to water ice, CO ice, and silicate dust in the spectrum of the bright infrared source (1RS 1) associated with the Herbig-Haro nebula HH 100 in the R Coronae Australis dark cloud. These absorptions are shown to arise predominantly in the...
Main Authors: | Whittet, D, Smith, R, Adamson, A, Aitken, D, Cihar, J, Kerr, T, Roche, P, Smith, C, Wright, C |
---|---|
Format: | Journal article |
Language: | English |
Published: |
Institute of Physics Publishing
1996
|
Similar Items
-
Interstellar dust absorption features in the infrared spectrum of HH 100-IR: Searching for the nitrogen component of the ices
by: Whittet, D, et al.
Published: (1996) -
Spectropolarimetric constraints on the nature of the 3.4 micron absorber in the interstellar medium
by: Adamson, A, et al.
Published: (1999) -
Spectropolarimetric constraints on the nature of the 3.4 micron absorber in the interstellar medium
by: Adamson, A, et al.
Published: (1999) -
Interstellar polarization from CO and XCN mantled grains: A severe test for grain alignment mechanisms
by: Chrysostomou, A, et al.
Published: (1996) -
Interstellar polarization from CO and XCN mantled grains: A severe test for grain alignment mechanisms
by: Chrysostomou, A, et al.
Published: (1996)