Interstellar Hydrocarbons is a class of organic molecules composed predominantly of hydrogen and carbon atoms that are formed and detected in the interstellar medium, distinguished by their spectroscopic signatures and role in the chemical evolution of space environments.
439
Publications
30.9K
Citations
1.2K
Authors
476
Institutions
Publications per year
2017–2026
87
Parents
Publications
439
A. G. G. M. Tielens · Reviews of Modern Physics · 2013 · 771 citations
Natural Sciences, Chemistry, Physics +17
1–5 of 439
Authors
1.2K
- LJ
28
h-index
- AG
25
h-index
- EH
16
h-index
- CJ
16
h-index
- RI
14
h-index
1–5 of 1.2K
Institutions
476
Ames Research Center
Mountain View, United States
38 h-index
139 publications
14K citations
Centre National de la Recherche Scientifique
Paris, France
34 h-index
166 publications
13K citations
Leiden University
Leiden, The Netherlands
25 h-index
92 publications
6.1K citations
Université Toulouse III - Paul Sabatier
Toulouse, France
19 h-index
52 publications
4.3K citations
Université Fédérale de Toulouse Midi-Pyrénées
Toulouse, France
17 h-index
38 publications
2.6K citations
Search for Extraterrestrial Intelligence
Mountain View, United States
17 h-index
27 publications
1.9K citations
Goddard Space Flight Center
Greenbelt, United States
17 h-index
37 publications
3.2K citations
Université Paris-Sud
Orsay, France
14 h-index
36 publications
5.7K citations
1–8 of 476
Venues
- The Astrophysical Journal
ApJ · 136 publications · 10.2K citations
60
h-index
- Astronomy and Astrophysics
46 publications · 3.4K citations
30
h-index
- Monthly Notices of the Royal Astronomical Society
32 publications · 801 citations
18
h-index
- Physical Chemistry Chemical Physics
PCCP · 13 publications · 563 citations
13
h-index
- Icarus
11 publications · 626 citations
11
h-index
1–5