Carbon monoxide is the second most abundant molecule in interstellar space
and therefore of key interest in astrophysics. In particular, the rate and
mechanism of photodissociation by vacuum ultraviolet (VUV) radiation have
been the subject of intensive spectroscopic investigations over the past
years. It is now a well-knon fact that CO is photodissociated by absorption
of VUV photons on discrete lines. The excited (Rydberg) states are mostly
predissociated through the interaction with continuum states.
While considerable data has been gathered on highly excited singlet states,
very little was known about their triplet counterparts. The reason, of
course, is that conventional absorption spectroscopy is of limited value for
the study of triplet states since the transitions from the
X 1Sigma+ ground state are spin-forbidden.
The multi-step excitation scheme
| j 3Sigma+ (v=0) | k 3Pi | |
| electronic and vibrational energy T | 90833.233(32) | 91959.354(24) |
| rotational constant B | 1.9381(12) | 1.2805(16) |
| spin-orbit interaction A | 29.953(14) | |
| spin-spin interaction lambda | -0.077(32) | 0.022(11) |
| spin-rotation interaction gamma | -0.091(21) | |
| lambda doubling p | 0.0 | |
| lambda doubling q | 0.0 |
RKR potential curves of CO near the dissociation threshold
Rydberg levels of carbon monoxide
© 1995 C.R.Vidal; E-mail: crv@mpe-garching.mpg.de
Last change: 28 June 1997