𝔖 Bobbio Scriptorium
✦   LIBER   ✦

A priori predictions of the rotational constants for HC13N, HC15N, and C5O

✍ Scribed by D.J. Defrees; A.D. McLean


Publisher
Elsevier Science
Year
1989
Tongue
English
Weight
426 KB
Volume
158
Category
Article
ISSN
0009-2614

No coin nor oath required. For personal study only.

✦ Synopsis


Ab initio molecular orbital theory is used to estimate the rotational constant for several carbon-chain molecules that are candidates for discovery in interstellar space. These estimated rotational constants can be used in laboratory or astronomical searches for the molecules. The rotatlonal constant for HCIJN is estimated to be 0.1073 kO.0002 GHz and its dipolc moment 5.4 D. The rotational constant for HClsN is estimated to be 0.0724 GHz,with a somewhat larger uncertainty. The rotational constant ofC@ is estimated to be 1.360 I!I 2% GHz and its dipole moment 4.4. D.


πŸ“œ SIMILAR VOLUMES


A priori predictions of the rotational c
✍ D.J. Defrees; A.D. McLean πŸ“‚ Article πŸ“… 1986 πŸ› Elsevier Science 🌐 English βš– 449 KB

Protonated formaldehyde and protonated methanol are candidate interstellar molecules and models for classes of protonatkd oxygen compounds. Ab initio molecular orbital theory has been used to compute rotational constants to guide spectroscopic searches both in the laboratory and in space. The ab tit

79Br-Nuclear quadrupole coupling in the
✍ A.C. Legon πŸ“‚ Article πŸ“… 1987 πŸ› Elsevier Science 🌐 English βš– 478 KB

The ground-state rotational spectrum of the linear, hydrogen-bonded isotopomer HC'5N...D79Br has been investigated by pulsednozzle Fourier-transform microwave spectroscopy to give the spectroscopic constants &= 1374.4429( 3) MHz, D,= 1.790( ) kHz, x( 79Br) =438.645( 9) MHz and M( 79Br) =2.4( 3) kHz.

Assignment of the relative configuration
✍ Jorge Antonio Guerrero-Alvarez; Antonio Moncayo-Bautista; Armando Ariza-Castolo πŸ“‚ Article πŸ“… 2004 πŸ› John Wiley and Sons 🌐 English βš– 171 KB

## Abstract The relative configuration of 11 1,4‐diazaspiro[4.5]decanes (**1a–1j** and **1m**), 15 1,4‐oxazaspiro[4.5]decanes (**2a–2o**) and 10 1,4‐dioxaspiro[4.5]decanes (**3a–3n**) substituted at the 2‐, 6‐, 7‐ or 8‐position by a methyl group or using the __tert__‐butyl group as a model for the