2005ApJ...619..939G


Query : 2005ApJ...619..939G

2005ApJ...619..939G - Astrophys. J., 619, 939-944 (2005/February-1)

The radio spectra of S3and S4.

GOTTLIEB C.A., THORWIRTH S., McCARTHY M.C. and THADDEUS P.

Abstract (from CDS):

The pure rotational spectra of the polar asymmetric top molecules S3 and S4have recently been observed in the laboratory for the first time. Approximately 150 transitions of S3between 10 and 458 GHz and a similar number for S4between 6 and 271 GHz have been measured. Many transitions of both molecules are accessible with existing telescopes across the entire radio band. The most interesting astronomical lines to 300 GHz are calculated here from the derived spectroscopic constants to an uncertainty of 1 km/s or better in equivalent radial velocity, and even at 700 GHz uncertainties are probably worse by only an order of magnitude. Both S3and S4are plausible candidates for detection in Galactic molecular sources, the atmosphere of the Jovian moon Io, and comets.

Abstract Copyright:

Journal keyword(s): ISM: Molecules - Molecular Data - Molecular Processes - Radio Lines: ISM - Stars: Formation

CDS comments: IRS 16293 = NAME IRAS 1629A

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1676 0
2 NAME OMC1 Ridge reg 05 35 13.4 -05 23 07           ~ 128 0
3 NAME Orion Core ? 05 35 14.5 -05 22 30           ~ 202 0
4 M 42 HII 05 35 17 -05 23.4           ~ 4078 0
5 NAME Ori A MoC 05 38 -07.1           ~ 3013 0
6 OH 231.8+04.2 OH* 07 42 16.947 -14 42 50.20           M10III+A 533 0
7 IRC +10216 C* 09 47 57.40632 +13 16 43.5648           C9,5e 2343 0
8 IRAS 16293-2422 cor 16 32 22.56 -24 28 31.8           ~ 1252 1
9 NAME Sgr B2 (North) Rad 17 47 20.2 -28 22 21           ~ 673 1
10 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2266 1
11 NAME Sgr B2 Main Rad 17 47 20.5 -28 23 06           ~ 407 1
12 NAME Sgr B2 (OH) MoC 17 47 20.8 -28 23 32           ~ 88 0

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