International audienceWe calculate collision strengths and their thermally-averaged Maxwellian values for electron excitation and de-excitation between the fifteen lowest levels of singly-ionized cobalt, Co+, which give rise to emission lines in the near- and mid-infrared. Transition probabilities are also calculated and relative line intensities predicted for conditions typical of supernova ejecta. The diagnostic potential of the 10.52, 15.46 and 14.74 μm transition lines is briefly discussed
This work reports new experimental radiative lifetimes and calculated oscillator strengths for trans...
We report the detection of far-infrared (FIR) CO rotational emission from nearby active galactic nuc...
We report the detection of eight high-N rotational transitions of CO+ towards a low mass protostar, ...
International audienceWe calculate collision strengths and their thermally-averaged Maxwellian value...
<p>We calculate collision strengths and their thermally-averaged Maxwellian values for electron exci...
In this paper we compute the collision strengths and their thermally-averaged Maxwellian values for ...
The list presents electron collision strengths for the forbidden transitions between the fifteen low...
The list presents electron collision strengths for the forbidden transitions between the fifteen low...
Radiative transition probabilities have been calculated for the magnetic dipole (M1) and electric qu...
Context. Observations of CO+ suggest column densities on the order 1012 cm-2 that can not be reprodu...
<p>We present effective collision strengths for electron excitation and de-excitation of the ten for...
We obtained optical and near infrared spectra of Type Ia supernovae (SNe Ia) at epochs ranging from ...
We present electron collision strengths and their thermally averaged values for the forbidden lines ...
This work reports new experimental radiative lifetimes and calculated oscillator strengths for tran...
Author Institution: Dept. of Physics, University of Toronto; Instytut Fizyki, Universytet Miko{\l}aj...
This work reports new experimental radiative lifetimes and calculated oscillator strengths for trans...
We report the detection of far-infrared (FIR) CO rotational emission from nearby active galactic nuc...
We report the detection of eight high-N rotational transitions of CO+ towards a low mass protostar, ...
International audienceWe calculate collision strengths and their thermally-averaged Maxwellian value...
<p>We calculate collision strengths and their thermally-averaged Maxwellian values for electron exci...
In this paper we compute the collision strengths and their thermally-averaged Maxwellian values for ...
The list presents electron collision strengths for the forbidden transitions between the fifteen low...
The list presents electron collision strengths for the forbidden transitions between the fifteen low...
Radiative transition probabilities have been calculated for the magnetic dipole (M1) and electric qu...
Context. Observations of CO+ suggest column densities on the order 1012 cm-2 that can not be reprodu...
<p>We present effective collision strengths for electron excitation and de-excitation of the ten for...
We obtained optical and near infrared spectra of Type Ia supernovae (SNe Ia) at epochs ranging from ...
We present electron collision strengths and their thermally averaged values for the forbidden lines ...
This work reports new experimental radiative lifetimes and calculated oscillator strengths for tran...
Author Institution: Dept. of Physics, University of Toronto; Instytut Fizyki, Universytet Miko{\l}aj...
This work reports new experimental radiative lifetimes and calculated oscillator strengths for trans...
We report the detection of far-infrared (FIR) CO rotational emission from nearby active galactic nuc...
We report the detection of eight high-N rotational transitions of CO+ towards a low mass protostar, ...