Identification of the emission feature near 3.5 microns in the pre-main-sequence star HD 97048-Reference-Cited by-同舟云学术

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Identification of the emission feature near 3.5 microns in the pre-main-sequence star HD 97048

Published:1983-02 Issue: Volume:265 Page:290
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Baas F.,Allamandola L. J.,Geballe T. R.,Persson S. E.,Lacy J. H.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 28 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Diamond phase in space and the possibility of its spectroscopic detection;Uspekhi Fizicheskih Nauk;2024-02

2. Diamond phase in space and the possibility of its spectroscopic detection;Physics-Uspekhi;2024-02

3. Nanodiamonds around HD 97048 and Elias 1;Astronomy & Astrophysics;2002-03

4. Detection of the unusual 3.5 μm feature in the Herbig Be star MWC 297;Astronomy & Astrophysics;2001-10

5. Diamond Infrared Emission Bands in Circumstellar Media;The Astrophysical Journal;1999-08-20

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