We report on the discovery of two new molecules, HCCCHCCC and HCCCCS, towards the starless core TMC-1 in the Taurus region from the QUIJOTE line survey in the 31.1-50.2 GHz frequency range. We identify a total of twenty-nine lines of HCCCHCCC and six rotational transitions of HCCCCS. The rotational quantum numbers range from Ju=10 up to 15 and Ka <=2 for HCCCHCCC and Ju=21/2 up to 31/2 for HCCCCS. We derived a column density for HCCCHCCC of N=(1.3+/-0.2)x10^11 cm-2 with a rotational temperature of 6+/-1 K, while for HCCCCS we derived N=(9.5+/-0.8)x10^10 cm-2 and Trot =10+/-1 K. The abundance of HCCCHCCC is higher than that of its recently discovered isomer, l-H2C6. If we compare HCCCCS with its related molecules, HCS and HCCS, we obtain abu...
The recent detection of the hydrocarbon anion C6H- in the interstellar medium has led us to investig...
We present the detection of two HCO isomers, propynal and cyclopropenone, toward various starless co...
The studies of the complex molecular emission lines in millimeter and submillimeter wavelengths towa...
Using the QUIJOTE line survey in the 32.0-50.4 GHz range, we report the discovery of the molecule CH...
We report on the discovery of two new molecules, HCCCHCCC and HCCCCS, towards the starless core TMC-...
Bell et al. reported the first detection of the cyanopolyyne HC_(11)N towards the cold dark cloud TM...
12 pags., 5 figs., 5 tabs.Using the QUIJOTE line survey in the 32.0-50.4 GHz range, we report the di...
We report the detection of large hydrocarbon cycles toward several cold dense clouds. We observed fo...
We report the discovery of five cyano derivatives of propene towards TMC-1 with the QUIJOTE line sur...
The recent interstellar detection of cyanonaphthalenes bring interest in related aromatic molecular ...
Author Institution: Chemical Physics Program, The Ohio State University, Columbus, OH 43210; Departm...
The previous detection of two species related to the non polar molecule cyanogen (NCCN), its protona...
The cumulene carbenes are important components of hydrocarbon chemistry in low-mass star-forming cor...
\begin{wrapfigure}{r}{0.5\textwidth} \vspace{-32pt} \begin{center} \includegraphics[width=0.40\tex...
We report new observations of molecular anions with the Yebes 40m and IRAM 30m telescopes toward the...
The recent detection of the hydrocarbon anion C6H- in the interstellar medium has led us to investig...
We present the detection of two HCO isomers, propynal and cyclopropenone, toward various starless co...
The studies of the complex molecular emission lines in millimeter and submillimeter wavelengths towa...
Using the QUIJOTE line survey in the 32.0-50.4 GHz range, we report the discovery of the molecule CH...
We report on the discovery of two new molecules, HCCCHCCC and HCCCCS, towards the starless core TMC-...
Bell et al. reported the first detection of the cyanopolyyne HC_(11)N towards the cold dark cloud TM...
12 pags., 5 figs., 5 tabs.Using the QUIJOTE line survey in the 32.0-50.4 GHz range, we report the di...
We report the detection of large hydrocarbon cycles toward several cold dense clouds. We observed fo...
We report the discovery of five cyano derivatives of propene towards TMC-1 with the QUIJOTE line sur...
The recent interstellar detection of cyanonaphthalenes bring interest in related aromatic molecular ...
Author Institution: Chemical Physics Program, The Ohio State University, Columbus, OH 43210; Departm...
The previous detection of two species related to the non polar molecule cyanogen (NCCN), its protona...
The cumulene carbenes are important components of hydrocarbon chemistry in low-mass star-forming cor...
\begin{wrapfigure}{r}{0.5\textwidth} \vspace{-32pt} \begin{center} \includegraphics[width=0.40\tex...
We report new observations of molecular anions with the Yebes 40m and IRAM 30m telescopes toward the...
The recent detection of the hydrocarbon anion C6H- in the interstellar medium has led us to investig...
We present the detection of two HCO isomers, propynal and cyclopropenone, toward various starless co...
The studies of the complex molecular emission lines in millimeter and submillimeter wavelengths towa...