The silicate absorption profile in the interstellar medium towards the heavily obscured nucleus of NGC 4418

The 9.7-...m silicate absorption profile in the interstellar medium (ISM) provides important information on the physical and chemical composition of interstellar dust grains. Measurements in the Milky Way have shown that the profile in the diffuse ISM is very similar to the amorphous silicate profil...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2015-05, Vol.449 (3), p.2598-2598
Main Authors: Roche, P F, Alonso-Herrero, A, Gonzalez-Martin, O
Format: Article
Language:English
Subjects:
Astronomy
Diffusion
Dust
Emission
Grains
Interstellar matter
Milky Way
Nuclei
Silicates
Silicon carbide
Star & galaxy formation
Symbols
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Summary:The 9.7-...m silicate absorption profile in the interstellar medium (ISM) provides important information on the physical and chemical composition of interstellar dust grains. Measurements in the Milky Way have shown that the profile in the diffuse ISM is very similar to the amorphous silicate profiles found in circumstellar dust shells around late M stars, and narrower than the silicate profile in denser star-forming regions. Here, we investigate the silicate absorption profile towards the very heavily obscured nucleus of NGC 4418, the galaxy with the deepest known silicate absorption feature, and compare it to the profiles seen in the Milky Way. Comparison between the 8-13 ...m spectrum obtained with Thermal-Region Camera Spectrograph on Gemini and the larger aperture spectrum obtained from the Spitzer archive indicates that the former isolates the nuclear emission, while Spitzer detects low surface brightness circumnuclear diffuse emission in addition. The silicate absorption profile towards the nucleus is very similar to that in the diffuse ISM in the Milky Way with no evidence of spectral structure from crystalline silicates or silicon carbide grains. (ProQuest: ... denotes formulae/symbols omitted.)
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stv495