1974
DOI: 10.1007/bf01732020
|View full text |Cite
|
Sign up to set email alerts
|

Hot hydrogen atoms reactions of interest in molecular evolution and interstellar chemistry

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
7
0

Year Published

1976
1976
2021
2021

Publication Types

Select...
8
1

Relationship

0
9

Authors

Journals

citations
Cited by 22 publications
(7 citation statements)
references
References 15 publications
0
7
0
Order By: Relevance
“…Nuevo et al (2008) were not able to confirm the synthesis of α-histidine and α-lysine in ISM experiments. It also should be pointed out that using reducing atmospheres Becker et al (1974) and RuizBermejo et al (2007) were able to show the synthesis of α-isoleucine, which it was not synthesized in the experiments of Table 1 or found in meteorites (Tables 2, 3, 4). This is an important issue since these amino acids (α-lysine, α-histidine, α-asparagine, α-isoleucine) play important roles in our biochemistry.…”
Section: Endogenous Amino Acidsmentioning
confidence: 91%
See 1 more Smart Citation
“…Nuevo et al (2008) were not able to confirm the synthesis of α-histidine and α-lysine in ISM experiments. It also should be pointed out that using reducing atmospheres Becker et al (1974) and RuizBermejo et al (2007) were able to show the synthesis of α-isoleucine, which it was not synthesized in the experiments of Table 1 or found in meteorites (Tables 2, 3, 4). This is an important issue since these amino acids (α-lysine, α-histidine, α-asparagine, α-isoleucine) play important roles in our biochemistry.…”
Section: Endogenous Amino Acidsmentioning
confidence: 91%
“…Miller (1953) was the first who showed that the synthesis of amino acids was possible from a mixture of gases. Table 5 shows several protein amino acids as well as non-protein amino acids that were synthesized in environments simulating the atmosphere of prebiotic earth (Janda et al 2008;Ruiz-Bermejo et al 2007;Plankensteiner et al 2006;Civiš et al 2004;Miyakawa et al 2002;Kobayashi et al 2001;Kobayashi et al 1999b;Miyakawa et al 1999;Takahashi et al 1999;Kobayashi et al 1998;Hirose et al 1990Hirose et al -1991Kobayashi et al 1990;Schlesinger and Miller 1983;Shimoyama et al 1978;Becker et al 1974;Sagan and Khare 1971;Bar-Nun et al 1970;Miller 1953).…”
Section: Sources Of Amino Acids On the Prebiotic Earthmentioning
confidence: 98%
“…The abiotic synthesis of Phe and Tyr occurs in a large variety of space and geochemical scenarios, including meteorite-catalyzed thermal processes [76], spark discharge in gas mixtures [77], associated with self-crystallization and racemic resolution [78], high pressure hydrothermal transformations [79], and the geological process of serpentinization [80], also focusing on the catalytic role of biomorph structures [81]. The possible prebiotic synthesis mechanisms for Cys include irradiation [82] and hydrothermal processes [83]. The latter mechanism is generally thought to involve so-called Strecker-cyanohydrin synthesis, a sequential chemical condensation of hydrogen cyanide (HCN) and aldehydes [84].…”
Section: Melanin-type Materials and Precursors In Astrochemical Environmentsmentioning
confidence: 99%
“…Many chemical reactions involving H atoms and important for interstellar chemical networks have a threshold that can be overcome by the availability of extra kinetic energy. Examples are the trapping of H atoms in solid hydrogen (Miyazaki et al 1983), the hydrogen abstraction from several molecules like H 2 O, H 2 S, hydrocarbons (Becker et al 1974) and their deuterated versions (Nicholas & Vaghjiani 1989;Malcolme-Lawes 1972), and the impact ionization of I group metals (Crooks et al 1978). It is therefore important to develop practical and reliable methods to characterize the chemical reactivity of H atoms after their production including the effects due to their moderation, thermalization, loss, and reactions with other species.…”
Section: Introductionmentioning
confidence: 99%