A λ2 mm molecular line survey of the C-star envelope IRC+10216

By J. Cernicharo, M. Guélin, C. Kahane. 2000

245 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/167f404dda209deafa8811efea3185d06ca2441e

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. H. Olofsson
2. C. Walsh
3. S. Höfner
4. È. Roueff
5. T. Millar
6. Michael C. McCarthy
7. P. Thaddeus
8. J. Cernicharo

In Atmospheric Science

1. T. Millar
2. J. Cernicharo
3. D. McElroy
4. Kenneth W. Smith
5. M. Cordiner
6. C. Walsh
7. A. Markwick
8. B. McGuire

In Spectroscopy

1. Michael C. McCarthy
2. M. Agúndez
3. T. Millar
4. J. Cernicharo
5. P. Thaddeus
6. S. García-Burillo
7. D. McElroy
8. Kenneth W. Smith

Citations in the corpus

• The UMIST database for astrochemistry 2012 (2012, background): “The cool, expanding outer envelope of the carbon-rich AGB star, IRC+10216, is one of the most important extra-terrestrial environments for the study of gasphase chemical kinetics due to the abundance and diversity of the different molecules detected in the envelope (e.g. Cernicharo et al. 2000).”
• Discovery of Interstellar Propylene (CH2CHCH3): Missing Links in Interstellar Gas-Phase Chemistry (2007, methodology): “Using the spectral line catalog developed and maintained at the DAMIR-IEM-CSIC (Cernicharo et al. 2000), we tentatively identified these two lines as one doublet arising from the (505 − 404) rotational transition (A and E species) of propylene (also called propene, CH2CHCH3) in the survey data of…”
• Mass loss of stars on the asymptotic giant branch (2018, background): “The molecular setups of O- and C-CSEs are markedly different (Cernicharo et al. 2000; Velilla Prieto et al. 2017), except for the fact that CO is the most abundant molecule (next to H2) in both cases (H2O may rival CO in O-CSEs).”
• A line confusion limited millimeter survey of Orion KL I. Sulfur carbon chains - I. Sulfur carbon chains (2010, methodology): “We applied this procedure to all our previous line surveys with the 30m telescope (e.g., Cernicharo et al. 2000).”
• A 2 Millimeter Spectral Line Survey of the Starburst Galaxy NGC 253 (2006, background): “…been the result of unbiased frequency scans toward specific Galactic sources, such as massive star-forming regions (e.g., Sgr B2(M), Cummins et al. 1986; OriMC-1, Lee et al. 2001), cold molecular clouds (e.g., TMC-1, Kaifu et al. 2004), and evolved stars (e.g., IRC +10216, Cernicharo et al. 2000).”
• Detection of C5N− and Vibrationally Excited C6H in IRC +10216 (2008, background): “The dusty envelope of the carbon star IRC+10216 is a rich radio source where at least 70 molecules have been observed (see, e.g., Cernicharo et al. 2000).”