Zobrazeno 1 - 10
of 206
pro vyhledávání: '"Müller, Holger S P"'
Autor:
Zingsheim, Oliver, Bonah, Luis, Lewen, Frank, Thorwirth, Sven, Müller, Holger S. P., Schlemmer, Stephan
Publikováno v:
J. Mol. Spectrosc. 381 (2021) 111519
A new millimeter- to millimeter-wave double-modulation double-resonance (MMW-MMW DM-DR) scheme has been applied to record spectra of two astronomically relevant complex organic molecules (COMs), propanal (C2H5CHO) and ethyl cyanide (C2H5CN), to demon
Externí odkaz:
http://arxiv.org/abs/2407.01297
Publikováno v:
A&A 688, A201 (2024)
Methanol is an abundant molecule in space. The column density of CH$_3^{18}$OH is in some star-forming regions so high that the search for CH$_3^{17}$OH is promising. But only very few transition frequencies of CH$_3^{17}$OH with a microwave accuracy
Externí odkaz:
http://arxiv.org/abs/2407.01139
Autor:
Sanz-Novo, Miguel, Rivilla, Víctor M., Müller, Holger S. P., Jiménez-Serra, Izaskun, Martín-Pintado, Jesús, Colzi, Laura, Zeng, Shaoshan, Megías, Andrés, López-Gallifa, Álvaro, Martínez-Henares, Antonio, Tercero, Belén, de Vicente, Pablo, Andrés, David San, Martín, Sergio, Requena-Torres, Miguel A.
We present the first detection in space of thionylimide (HNSO) toward the Galactic Center molecular cloud G+0.693-0.027, thanks to the superb sensitivity of an ultradeep molecular line survey carried out with the Yebes 40$\,$m and IRAM 30$\,$m telesc
Externí odkaz:
http://arxiv.org/abs/2404.01044
Publikováno v:
Astron. Astrophys. 681 (2024) A104
We want to investigate the influence of the powerful outflow driven by the hot core Sgr B2(N1) on the gas molecular inventory of the surrounding medium. We used the data taken as part of the 3 mm imaging spectral-line survey ReMoCA (Re-exploring Mole
Externí odkaz:
http://arxiv.org/abs/2310.11339
Autor:
Fatima, Mariyam, Müller, Holger S. P., Zingsheim, Oliver, Lewen, Frank, Rivilla, Víctor M., Jiménez-Serra, Izaskun, Martín-Pintado, Jesús, Schlemmer, Stephan
Publikováno v:
A&A 680, A25 (2023)
Isobutene ((CH$_3$)$_2$C=CH$_2$) is one of the four isomers of butene (C$_4$H$_8$). Given the detection of propene (CH$_3$CH=CH$_2$) toward TMC-1, and also in the warmer environment of the solar-type protostellar system IRAS 16293$-$2422, one of the
Externí odkaz:
http://arxiv.org/abs/2309.17236
Autor:
Müller, Holger S. P., Maeda, Atsuko, Lewen, Frank, Schlemmer, Stephan, Medvedev, Ivan R., Herbst, Eric
Publikováno v:
Mol. Phys. 122 (2024) e2262057
An investigation of the rotational spectrum of the interstellar molecule thioformaldehyde between 110 and 377 GHz through a pyrolysis reaction revealed a multitude of absorption lines assignable to H$_2$CS and H$_2$C$^{34}$S in their lowest four exci
Externí odkaz:
http://arxiv.org/abs/2309.08992
Autor:
Müller, Holger S. P., Jørgensen, Jes K., Guillemin, Jean-Claude, Lewen, Frank, Schlemmer, Stephan
Publikováno v:
J. Mol. Spectrosc. 394 (2023) 111777
We prepared a sample of oxirane doubly deuterated at one C atom and studied its rotational spectrum in the laboratory for the first time between 120~GHz and 1094~GHz. Accurate spectroscopic parameters up to eighth order were determined, and the calcu
Externí odkaz:
http://arxiv.org/abs/2304.12045
Autor:
Müller, Holger S. P., Jørgensen, Jes K., Guillemin, Jean-Claude, Lewen, Frank, Schlemmer, Stephan
Publikováno v:
Mon. Not. R. Astron. Soc., 518, 185-193 (2023)
We prepared a sample of mono-deuterated oxirane and studied its rotational spectrum in the laboratory between 490 GHz and 1060 GHz in order to improve its spectroscopic parameters and consequently the calculated rest frequencies of its rotational tra
Externí odkaz:
http://arxiv.org/abs/2209.01414
Autor:
Bonah, Luis, Zingsheim, Oliver, Müller, Holger S. P., Guillemin, Jean-Claude, Lewen, Frank, Schlemmer, Stephan
Acetone-13C1 is a complex organic molecule with two internal methyl (-CH3) rotors having relatively low effective barriers to internal rotation of about 249 cm-1. This leads to two low-lying torsional modes and five internal rotation components resul
Externí odkaz:
http://arxiv.org/abs/2207.13953
Publikováno v:
A&A 665, A96 (2022)
Using the high angular resolution provided by the ALMA interferometre we want to resolve the COM emission in the hot molecular core Sagittarius B2(N1) and thereby shed light on the desorption process of Complex Organic Molecules (COMs) in hot cores.
Externí odkaz:
http://arxiv.org/abs/2206.11174