Title: Submillimeterwave Spectroscopy of 13C1Methyl formate H13COOCH3 in the Ground State
1Submillimeter-wave Spectroscopy of13C1-Methyl
formate H13COOCH3in the Ground State
- Atsuko Maeda, Ivan Medvedev,
- Eric Herbst, Frank C. De Lucia,
- Department of Physics, The Ohio State University,
Columbus, OH - and Peter Groner
- Department of Chemistry, University of
Missouri-Kansas City, Kansas City, MO
2(Normal) Methyl formate
- One of abundant interstellar molecules
- in hot cores corinos (Orion KL, Sgr B2)
T 100-300 K
Ultra-compact HII region
O,B star
n 10(6)-10(8) cm-3
Cold background
Hot Core
3CH3 Internal Rotationin Methyl formate
with ZPVE (zero-point vibrational correction)
E
407 MHz (0.0135 cm-1)
A
Senent, Villa, Meléndez and Dominguez-Gomez, ApJ.
627, 567 (2005)
4Previous Rotational Studies of Methyl formate
- Curl (1959) - HCOOCH3, DCOOCH3, HCOOCH2D,
H13COOCH3, HCOO13CH3, - HC18OOCH3, HCO18OCH3 10-30 GHz vt 0 (A, E),
HR - Bauer (1979) - HCOOCH3 5-58 GHz vt 0 (A, E),
IAM - DeMaison et al. (1983) - HCOOCH3 220-240 GHz
vt 0 (A, E) - Plummer et al. (1984) - HCOOCH3 140-550 GHz vt
0 (A), HR - Plummer et al. (1986) - HCOOCH3 140-300 GHz vt
0 (E), PAM - Oesterling et al. (1995) - DCOOCH3 -680 GHz vt
0 (A, E), RAM - Oesterling et al. (1999) - HCOOCH3 -380 GHz vt
0 (A, E), RAM - Karakawa et al. (2001) - HCOOCH3
- Odashima et al. (2003) - HCOOCH3 7-200 GHz vt
0 (A, E), 1 (A), IAM
Fewer studies for isotopologues
5Previous Study of 13C1-Methyl formate
- Willaert et al. (2006)
- 7-62, 300-322 570-610 GHz
- Ground A, E states
- Jmax 58 (Kmax 24)
- RAM Hamiltonian
13C
A few b-type transitions No prediction
Detection in interstellar media??
Willaert et al. J. Mol. Struct., 795, 4 (2006)
6Experiment
- FASSST spectrometer at OSU
- 110-380 GHz with three BWOs
- 100 scans accumulation
- up down-ward sweeps ? averaged
- SO2 lines ring cavity for frequency calibration
- Commercial H13COOCH3
- (Cambridge Isotope Laboratories, Inc.)
- A few mTorr in 8 m-long aluminum cell
- under room temperature
7FASSST Spectrum of 13C1-Methyl formate
9000 lines with S/N gt 5
CAAARS(1) (Computer Aided Assignment of
Asymmetric Rotor Spectra)
(1) Medvedev et al. J. Mol. Struct. 742, 299
(2005)
8Spectrum of 13C1-Methyl formate
9Transitions of 13C1-Methyl formate
a, b-type R, Q, P transitions c-type R, Q
x-type R transitions
1900 lines ? 2200 A transitions 2200 lines ? 2300
E transitions
10Effective Rotational Hamiltonian (ErHam) by
GronerPeter Groner, J. Chem. Phys. 107, 4483
(1997)
- Developed for dual or single internal rotors
- dimethyl-ether, 3-methyl-1,2-butadiene, aceton,
ethyl methyl ether, dimethyl diselenide, methyl
cabamate etc. - Principal axes system (PAS) or
- Rho axis system (RAS)
- Torsional energy, rotational constants are given
as Fourier series
11Effective Hamiltonianbased on principal axes
system
Hrot for asymmetric rotor
Coriolis interaction
negligible
Torsional energy
where
12Molecular Constants of 13C1-Methyl formate
53 parameters for A E substates (4800 lines)
with RMS 90 kHz
Comparable with Willaert et al. (2006)
Prediction for astronomical observation
13Systematic Deviations at Low Ka
Perturbation at Ka 0, 1 hardly
happens perturbation at high J / Ka
affects through least-square fitting
A substate
E substate
Q-branch transitions (Ka 0, 1)
14Perturbation at High Ka
Single state analysis of the A state with a
rotational Hamiltonian for asymmetric-top rotors
R branch transitions in the A substate
15Perturbation?
- Perturbation partner
- CH3 torsion (? 130 cm-1)
- COC bending (? 318 cm-1)
- CO torsion (? 332 cm-1)
- No ?v?0 interaction in the ErHam
- Van Vleck transformation?
- Too close to use
- ?? interaction term directly
Ka gt 15
16Conclusions
- 3000 lines in 110-380 GHz were newly assigned to
4800 transitions of 13C1-methyl formate in the
ground state. - Most of transitions were fitted satisfactorily
within 100 kHz. - Perturbation from excited torsional states?
- Prediction of transition frequencies of
13C1-methyl formate has been made. - The first excited torsional state of 13C1-methyl
formate is now being investigated.