The hot core towards the intermediate mass protostar NGC7129 FIRS 2: Chemical similarities with Orion KL
arXiv:1405.4639 · doi:10.1051/0004-6361/201323074
Abstract
NGC 7129 FIRS 2 (hereafter FIRS 2) is an intermediate-mass (2 to 8 Msun) protostar located at a distance of 1250 pc. High spatial resolution observations are required to resolve the hot core at its center. We present a molecular survey from 218200 MHz to 221800 MHz carried out with the IRAM Plateau de Bure Interferometer. These observations were complemented with a long integration single-dish spectrum taken with the IRAM 30m telescope. We used a Local Thermodynamic Equilibrium (LTE) single temperature code to model the whole dataset. The interferometric spectrum is crowded with a total of ~300 lines from which a few dozens remain unidentified yet. The spectrum has been modeled with a total of 20 species and their isomers, isotopologues and deuterated compounds. Complex molecules like methyl formate (CH3OCHO), ethanol (CH3CH2OH), glycolaldehyde (CH2OHCHO), acetone (CH3COCH3), dimethyl ether (CH3OCH3), ethyl cyanide (CH3CH2CN) and the aGg' conformer of ethylene glycol (aGg'-(CH2OH)_2) are among the detected species. The detection of vibrationally excited lines of CH3CN, CH3OCHO, CH3OH, OCS, HC3N and CH3CHO proves the existence of gas and dust at high temperatures. In fact, the gas kinetic temperature estimated from the vibrational lines of CH3CN, ~405 K, is similar to that measured in massive hot cores. Our data allow an extensive comparison of the chemistry in FIRS~2 and the Orion hot core. We find a quite similar chemistry in FIRS 2 and Orion. Most of the studied fractional molecular abundances agree within a factor of 5. Larger differences are only found for the deuterated compounds D2CO and CH2DOH and a few molecules (CH3CH2CN, SO2, HNCO and CH3CHO). Since the physical conditions are similar in both hot cores, only different initial conditions (warmer pre-collapse phase in the case of Orion) and/or different crossing time of the gas in the hot core can explain this behavior.
arXiv comment30 pages, 9 figures
References in corpus (22)
- The Spitzer ice legacy: Ice evolution from cores to protostars
- Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)
- PROSAC: A Submillimeter Array Survey of Low-Mass Protostars. I. Overview of Program: Envelopes, Disks, Outflows and Hot Cores
- Complex molecules in the hot core of the low mass protostar NGC1333-IRAS4A
- The largest oxigen bearing organic molecule repository
- Hot corinos in NGC1333-IRAS4B and IRAS2A
- A line confusion limited millimeter survey of Orion KL (I): sulfur carbon chains
- Discovery of Fulminic Acid, HCNO, in Dark Clouds
- An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry
- Submm line imaging of Orion-KL with the Submillimeter Array
- First detection of doubly deuterated hydrogen sulfide
- CH3OCH3 in Orion-KL: a striking similarity with HCOOCH3
- ALMA 690 GHz observations of IRAS 16293-2422B: Infall in a highly optically-thick disk
- Submillimeter Array 440m/690GHz line and continuum observations of Orion-KL
- Detection of a hot core in the intermediate-mass (IM) Class 0 protostar NGC 7129--FIRS2
- A combined IRAM and Herschel/HIFI study of cyano(di)acetylene in Orion KL: tentative detection of DC3N
- IRAS 22198+6336: Discovery of an Intermediate-Mass Hot Core
- The IC1396N proto-cluster at a scale of 250 AU
- Extended warm gas in Orion KL as probed by methyl cyanide
- Herschel-PACS spectroscopy of the intermediate mass protostar NGC7129 FIRS 2
- Dissecting an intermediate-mass (IM) protostar: Chemical differentiation in IC1396N
- TIMASSS : The IRAS16293-2422 Millimeter And Submillimeter Spectral Survey: Tentative Detection of Deuterated Methyl Formate (DCOOCH3)
Cited by in corpus (12)
- Constraining the abundances of complex organics in the inner regions of solar-type protostars
- The ALMA-PILS survey: First detections of ethylene oxide, acetone and propanal toward the low-mass protostar IRAS 16293-2422
- Deuteration and evolution in the massive star formation process: the role of surface chemistry
- Detection of glycolaldehyde towards the solar-type protostar NGC1333 IRAS2A
- Gas-phase formation of acetaldehyde: review and new theoretical computations
- Prestellar grain-surface origins of deuterated methanol in comet 67P/Churyumov-Gerasimenko
- First Hot Corino detected around an Isolated Intermediate-Mass Protostar: Cep\,E-mm
- Oxygen atom reactions with C2H6, C2H4, and C2H2 in ices
- Formation of complex organic molecules in molecular clouds: acetaldehyde, vinyl alcohol, ketene, and ethanol via the "energetic" processing of CH ice
- Chemical modelling of glycolaldehyde and ethylene glycol in star-forming regions
- Probing the kinematics and chemistry of the hot core Mon R 2 IRS 3 using ALMA observations
- Sulphur-Bearing and Complex Organic Molecules in an Infrared Cold Core