Hot Organic Molecules toward a Young Low-Mass Star: A Look at Inner Disk Chemistry-Reference-Cited by-同舟云学术

Hot Organic Molecules toward a Young Low-Mass Star: A Look at Inner Disk Chemistry

Published:2005-12-28 Issue:2 Volume:636 Page:L145-L148
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Lahuis F.,van Dishoeck E. F.,Boogert A. C. A.,Pontoppidan K. M.,Blake G. A.,Dullemond C. P.,Evans II N. J.,Hogerheijde M. R.,Jørgensen J. K.,Kessler-Silacci J. E.,Knez C.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference36 articles.

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2. High-Resolution 4.7 Micron Keck/NIRSPEC Spectroscopy of the CO Emission from the Disks Surrounding Herbig Ae Stars

3. ISOCAM observations of the $\mathsf{\rho}$ Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster

4. Gas-phase CO$_\mathsf{2}$ toward massive protostars

5. CO Emission from Disks around AB Aurigae and HD 141569: Implications for Disk Structure and Planet Formation Timescales

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