Abundant Carbon-Chain Molecules toward the Low-Mass Protostar IRAS 04368+2557 in L1527

By N. Sakai, T. Sakai, T. Hirota, S. Yamamoto. 2008

158 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/f1085da9ffb8b64dd693f373b848dd068fada72a

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. P. Caselli
2. Cecilia Ceccarelli
3. R. Garrod
4. E. Herbst
5. V. Wakelam
6. K. Oberg
7. E. Bergin
8. A. Vasyunin

In Atomic and Molecular Physics, and Optics

1. P. Caselli
2. Cecilia Ceccarelli
3. R. Garrod

In Spectroscopy

1. P. Caselli
2. Cecilia Ceccarelli
3. R. Garrod
4. E. Herbst
5. K. Oberg
6. E. Bergin
7. V. Wakelam
8. A. Vasyunin

Citations in the corpus

• Our astrochemical heritage (2012, background): “Therefore, the presence of a WCCC zone may be a signature of fast collapse (Sakai et al. 2008), for example triggered by a shock from a nearby forming star or two encountering diffuse clouds.”
• A THREE-PHASE CHEMICAL MODEL OF HOT CORES: THE FORMATION OF GLYCINE (2013, background): “…chemistry associated with methane evaporation is often labeled warm carbon-chain chemistry (WCCC), and has been identified observationally by Sakai et al. (2008); however, it is unlikely that the enhancement in propionaldehyde seen in the models would be observable at the low abundances…”