On the methylacetylene abundance and nitrogen isotope ratio in Pluto’s atmosphere-Reference-Cited by-同舟云学术

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On the methylacetylene abundance and nitrogen isotope ratio in Pluto’s atmosphere

Published:2020-11 Issue: Volume:192 Page:105044
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Krasnopolsky Vladimir A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference48 articles.

1. On the ionospheric structure of Titan;Agren;Planet. Space Sci.,2009

2. Chemical Kinetics and Data for Use in Atmospheric Studies. Evaluation Number 18;Burkholder,2015

3. NIST-JANAF thermodynamic tables, 4th ed;Chase;J. Phys. Chem. Ref. Data. Monogr,1998

4. Haze in Pluto’s atmosphere;Cheng;Icarus,2017

5. Pluto’s atmosphere from stellar occultations in 2012 and 2013;Dias-Oliveira;Astrophys. J.,2015

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1. Russian Studies of Planetary Atmospheres in 2019–2022;Izvestiya, Atmospheric and Oceanic Physics;2023-12

2. Triton's photochemical model: Update;Icarus;2023-12

3. Planetary Atmosphere Studies in Russia in 2019–2022;Известия Российской академии наук. Физика атмосферы и океана;2023-12-01

4. N2 accretion, metamorphism of organic nitrogen, or both processes likely contributed to the origin of Pluto's N2;Icarus;2023-11

5. Pluto’s atmosphere observations with ALMA: Spatially-resolved maps of CO and HCN emission and first detection of HNC;Icarus;2022-01

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