Add to ORKGTheoretical rate constants are presented for excitation of NH3 by collisions with He. The lowest 22 levels of ortho-NH3 and the lowest 16 levels of para-NH3 are considered at kinetic temperatures of 15 to 300 K
The formalism for describing rotational excitation in collisions between symmetric top rigid rotors ...
L'observation et l'étude des milieux moléculaires tel que le milieu interstellaire requièrent une co...
The availability of collisional rate coefficients with H_2 is a pre-requisite for interpretation of ...
International audienceAbstract Ammonia (NH3) is the first polyatomic molecule detected in the inters...
Ammonia is one of the most widely observed molecules in space, and many observations are able to res...
International audienceAmmonia inversion lines are often used as probes of the physical conditions in...
Context.Observations of deuterated molecules are useful probes of the physical and chemical conditio...
International audienceContext: .Observations of deuterated molecules are useful probes of the physic...
Rates for rotational excitation of HC3N by collisions with He atoms and H2 molecules are computed fo...
International audienceWe present quantal close coupling (CC) calculations of rotational excitation r...
Observation and study of molecular clouds of the interstellar medium require knowledge of fundamenta...
International audienceAccurate estimation of the abundance of the NH 2 radical in the interstellar m...
Observation and study of interstellar molecular clouds require the knowledge of molecular data to de...
The availability of collisional rate coefficients is a prerequisite for an accurate interpretation o...
Collisional energy transfer of NH2 in its electronically excited state (A) over tilde (2)A(1) is inv...
The formalism for describing rotational excitation in collisions between symmetric top rigid rotors ...
L'observation et l'étude des milieux moléculaires tel que le milieu interstellaire requièrent une co...
The availability of collisional rate coefficients with H_2 is a pre-requisite for interpretation of ...
International audienceAbstract Ammonia (NH3) is the first polyatomic molecule detected in the inters...
Ammonia is one of the most widely observed molecules in space, and many observations are able to res...
International audienceAmmonia inversion lines are often used as probes of the physical conditions in...
Context.Observations of deuterated molecules are useful probes of the physical and chemical conditio...
International audienceContext: .Observations of deuterated molecules are useful probes of the physic...
Rates for rotational excitation of HC3N by collisions with He atoms and H2 molecules are computed fo...
International audienceWe present quantal close coupling (CC) calculations of rotational excitation r...
Observation and study of molecular clouds of the interstellar medium require knowledge of fundamenta...
International audienceAccurate estimation of the abundance of the NH 2 radical in the interstellar m...
Observation and study of interstellar molecular clouds require the knowledge of molecular data to de...
The availability of collisional rate coefficients is a prerequisite for an accurate interpretation o...
Collisional energy transfer of NH2 in its electronically excited state (A) over tilde (2)A(1) is inv...
The formalism for describing rotational excitation in collisions between symmetric top rigid rotors ...
L'observation et l'étude des milieux moléculaires tel que le milieu interstellaire requièrent une co...
The availability of collisional rate coefficients with H_2 is a pre-requisite for interpretation of ...