nsl call ic or is o for n imp hydro oly-ato chmar 1,2]. T sion in ium (ISM). This small molecule is potentially involved in the formation of more complex molecules such as carbon chains and carbonaceous circumstellar grains, and as a photo-fragment of polycyclic aromatic hydrocarbons (PAHs) [8,9]. Different from most asymmetric carbon-chain species, C3 cannot be detected in the interstellar medium by radio astronomy due to the lack of a u g 3,23–26]. Detailed 00–000 b menon in t 00 state were found by McCall et al. [23] in laboratory work and la plained in a perturbation model by Zhang et al. [24]. Ho the recent observation of a high resolution spectrum towards HD 169454 indicates that this model still does not fully explain the astronomica...
We report the detection of the elusive carbon-chain radical C5N in the dark cloud TMC1 and its tenta...
Small carbon chain molecules like linear C$_3$ are thought to play a crucial role in the formation o...
Abstract. The mm-wave spectrum of the C-star envelope IRC+10216 has been continuously surveyed betwe...
The A 1u X 1þg transition of the simplest polyatomic carbon chain molecule, C3, at 4051.6 A ̊ has be...
The tricarbon C3 molecule has been detected in a number of translucent interstellar clouds via its A...
Abstract. The tricarbon C3 molecule has been detected in a number of translucent interstellar clouds...
Author Institution: I. Physikalisches Institut, Universitat zu Koln, 50937 Koln, Germany; Karlsruher...
The mm-wave spectrum of the C-star envelope IRC+10216 has been continuously surveyed between 129.0 a...
Short carbon chains are fundamental for the chemistry of stellar and interstellar ambiences. The lin...
A new, very sensitive search for interstellar triatomic carbon has resulted in upper limits for a fe...
Vibration-rotation lines of C(3) have been identified in the circumstellar spectrum of the obscured ...
The carbon-star envelope IRC +10216 harbors a rich variety of molecules, with more than 80...
Cyclic species in the interstellar medium have been searched for almost since the first detection of...
The carbon-star envelope IRC +10216 harbors a rich variety of molecules, with more than 80 detected ...
The discovery of a strong microwave (1.6 cm-wavelength) spectral line, the carrier of which is commo...
We report the detection of the elusive carbon-chain radical C5N in the dark cloud TMC1 and its tenta...
Small carbon chain molecules like linear C$_3$ are thought to play a crucial role in the formation o...
Abstract. The mm-wave spectrum of the C-star envelope IRC+10216 has been continuously surveyed betwe...
The A 1u X 1þg transition of the simplest polyatomic carbon chain molecule, C3, at 4051.6 A ̊ has be...
The tricarbon C3 molecule has been detected in a number of translucent interstellar clouds via its A...
Abstract. The tricarbon C3 molecule has been detected in a number of translucent interstellar clouds...
Author Institution: I. Physikalisches Institut, Universitat zu Koln, 50937 Koln, Germany; Karlsruher...
The mm-wave spectrum of the C-star envelope IRC+10216 has been continuously surveyed between 129.0 a...
Short carbon chains are fundamental for the chemistry of stellar and interstellar ambiences. The lin...
A new, very sensitive search for interstellar triatomic carbon has resulted in upper limits for a fe...
Vibration-rotation lines of C(3) have been identified in the circumstellar spectrum of the obscured ...
The carbon-star envelope IRC +10216 harbors a rich variety of molecules, with more than 80...
Cyclic species in the interstellar medium have been searched for almost since the first detection of...
The carbon-star envelope IRC +10216 harbors a rich variety of molecules, with more than 80 detected ...
The discovery of a strong microwave (1.6 cm-wavelength) spectral line, the carrier of which is commo...
We report the detection of the elusive carbon-chain radical C5N in the dark cloud TMC1 and its tenta...
Small carbon chain molecules like linear C$_3$ are thought to play a crucial role in the formation o...
Abstract. The mm-wave spectrum of the C-star envelope IRC+10216 has been continuously surveyed betwe...