One hundred and fifty-three diatomic molecules, molecular ions, and radicals of astrophysical interest

1987 ◽  
Vol 135 (1) ◽  
pp. 1-74 ◽  
Author(s):  
Markandey Singh ◽  
Jai Prakash Chaturvedi
1989 ◽  
Vol 162 (2) ◽  
pp. 251-278 ◽  
Author(s):  
Markandey Singh ◽  
Jai Prakash Chaturvedi

1988 ◽  
Vol 128 ◽  
Author(s):  
G. F. Cerofolini ◽  
L. Meda ◽  
C. Volpones

ABSTRACTThis paper deals with the implantation of molecular ions in silicon. The ‘molecular’ effect, i.e. the increase of the displacement yield compared with the sum of the atomic yields, is weak for light molecules (e.g., H2) and for heavy diatomic molecules (e.g., Sb2 and Bi2), but, for instance, it is strong for C6H6 at energy per atomic mass of the order of 1 keV/amu. Binary collision calculations are used to give a pictorial view of the phenomena occurring along the ion path, and to predict superadditivity and damage columnarity. The increase of pressure and temperature to extreme conditions by implantation of molecular ions is discussed.


2006 ◽  
Vol 39 (19) ◽  
pp. S1241-S1258 ◽  
Author(s):  
B Roth ◽  
P Blythe ◽  
H Daerr ◽  
L Patacchini ◽  
S Schiller

1987 ◽  
Vol 120 ◽  
pp. 91-92 ◽  
Author(s):  
T. K. Balasubramanian ◽  
G. L. Bhale ◽  
Sheila Gopal ◽  
G. Krishnamurthy ◽  
G. Lakshminarayana ◽  
...  

Laboratory studies have been made on molecules of astrophysical interest such as AlO, CO, CrO, SiS, NH+ and OH. Vibrational and rotational constants have been determined more accurately in the various electronic states.


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