The nature of molecular cloud material in interplanetary dust

By L. Keller, S. Messenger, G. Flynn, S. Clemett, Sue Wirick, Chris Jacobsen. 2004

170 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/68a2a17e83ce9e05cdbc6d6ad60c8dd23d33a0b5

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Cecilia Ceccarelli
2. P. Caselli
3. A. Nguyen
4. P. Hoppe
5. S. Sandford
6. L. Nittler
7. E. Herbst
8. M. Tafalla

In Spectroscopy

1. Cecilia Ceccarelli
2. P. Caselli
3. S. Sandford
4. L. Nittler

Citations in the corpus

• Quantitative organic and light‐element analysis of comet 81P/Wild 2 particles using C‐, N‐, and O‐μ‐XANES (2008, background): “It is worth noting, however, that while this IDP clearly has not suffered any aqueous alteration since its formation, it has undergone mild thermal processing during atmospheric entry (Flynn et al. 2003; Keller et al. 2004).”
• Our astrochemical heritage (2012, background): “Similarly, IDPs contain about 10-12 % carbon, mostly in organic material, including aromatic and aliphatic compounds ([420]; [243]).”
• Ultra-primitive interplanetary dust particles from the comet 26P/Grigg–Skjellerup dust stream collection (2009, background): “Generally, D hotspots are associated with poorly ordered aliphatic carbon (Keller et al., 2004).”