Further infrared studies of the pre-main-sequence object HD 97048
Open Access
- 1 September 1981
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 196 (1) , 39P-44P
- https://doi.org/10.1093/mnras/196.1.39p
Abstract
8–13 µm spectrophotometry of HD 97048 has been obtained, following the discovery of a new narrow emission feature at 3.5 µm by Blades & Whittet. The spectrum shows the familiar but unidentified emission feature at 11.25 µm superimposed on a hot grey continuum. The failure to detect other emission structure in this window rules out polyoxymethylene as the source of the 3.5 µm feature. The relationship with the associated reflection nebula is discussed.Keywords
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