Detection of methyl isocyanate (CH3NCO) in a solar-type protostar-Reference-Cited by-同舟云学术

Detection of methyl isocyanate (CH3NCO) in a solar-type protostar

Author:

Martín-Doménech R.¹,Rivilla V. M.²,Jiménez-Serra I.³,Quénard D.³,Testi L.²⁴⁵,Martín-Pintado J.¹

Affiliation:

1. Centro de Astrobiología (INTA-CSIC), Ctra de Ajalvir, Km. 4, Torrejón de Ardoz, E-28850 Madrid, Spain

2. INAF/Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Florence, Italy

3. School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, UK

4. ESO/European Southern Observatory, Karl Schwarzschild str. 2, D-85748 Garching, Germany

5. Excellence Cluster ‘Universe’, Boltzmann str. 2, D-85748 Garching bei Muenchen, Germany

Funder

MINECO

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference36 articles.

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