High Resolution Laboratory Spectroscopy
arXiv:1605.07456 · doi:10.1051/eas/1575061
Abstract
In this short review we will highlight some of the recent advancements in the field of high-resolution laboratory spectroscopy that meet the needs dictated by the advent of highly sensitive and broadband telescopes like ALMA and SOFIA. Among these is the development of broadband techniques for the study of complex organic molecules, like fast scanning conventional absorption spectroscopy based on multiplier chains, chirped pulse instrumentation, or the use of synchrotron facilities. Of similar importance is the extension of the accessible frequency range to THz frequencies, where many light hydrides have their ground state rotational transitions. Another key experimental challenge is the production of sufficiently high number densities of refractory and transient species in the laboratory, where discharges have proven to be efficient sources that can also be coupled to molecular jets. For ionic molecular species sensitive action spectroscopic schemes have recently been developed to overcome some of the limitations of conventional absorption spectroscopy. Throughout this review examples demonstrating the strong interplay between laboratory and observational studies will be given.
arXiv commentProceedings of "The 6th Zermatt ISM Symposium: Conditions and Impact of Star Formation - From Lab to Space"
References in corpus (21)
- Detection of a branched alkyl molecule in the interstellar medium: iso-propyl cyanide
- Detection of a Noble Gas Molecular Ion, {36}ArH^+, in the Crab Nebula
- Sensitive Chiral Analysis via Microwave Three-wave Mixing
- The IRAM-30m line survey of the Horsehead PDR: II. First detection of the l-C3H+ hydrocarbon cation
- Ubiquitous argonium (ArH) in the diffuse interstellar medium -- a molecular tracer of almost purely atomic gas
- Detection of E-cyanomethanimine towards Sagittarius B2(N) in the Green Bank Telescope PRIMOS Survey
- The Detection of Interstellar Ethanimine (CH3CHNH) from Observations taken during the GBT PRIMOS Survey
- Hydrides in Young Stellar Objects: Radiation tracers in a protostar-disk-outflow system
- Pure rotational spectra of TiO and TiO_2 in VY Canis Majoris
- Discovery of interstellar mercapto radicals (SH) with the GREAT instrument on SOFIA
- High-Accuracy Quartic Force Field Calculations for the Spectroscopic Constants and Vibrational Frequencies of 1 ^1A' l-C3H-: A Possible Link to Lines Observed in the Horsehead Nebula PDR
- Detection of extragalactic argonium, ArH, toward PKS~1830211
- Spectroscopic Constants and Vibrational Frequencies for l-C3H+ and Isotopologues from Highly-Accurate Quartic Force Fields: The Detection of l-C3H+ in the Horsehead Nebula PDR Questioned
- Rotational spectroscopy, dipole moment and N nuclear hyperfine structure of -propyl cyanide
- ALMA observations of TiO around VY Canis Majoris
- Excitation and Abundance of C3 in star forming cores:Herschel/HIFI observations of the sight-lines to W31C and W49N
- The quest for complex molecules in space: Laboratory spectroscopy of n-butyl cyanide, n-C4H9CN, in the millimeter wave region and its astronomical search in Sagittarius B2(N)
- Detection of OD towards the low-mass protostar IRAS16293-2422
- Herschel Planetary Nebula Survey (HerPlaNS) - First Detection of OH+ in Planetary Nebulae
- Laboratory spectroscopy of 1,2-propanediol at millimeter and submillimeter wavelengths
- High Resolution Laboratory Spectroscopy