Zobrazeno 1 - 10
of 46
pro vyhledávání: '"Moeller, Th"'
Autor:
Hsieh, T. -H., Pineda, J. E., Segura-Cox, D. M., Caselli, P., Valdivia-Mena, M. T., Gieser, C., Maureira, M. J., Lopez-Sepulcre, A., Bouscasse, L., Neri, R., Möller, Th., Dutrey, A., Fuente, A., Semenov, D., Chapillon, E., Cunningham, N., Henning, Th., Pietu, V., Jimenez-Serra, I., Marino, S., Ceccarelli, C.
Publikováno v:
A&A 686, A289 (2024)
Complex Organic Molecules (COMs) have been found toward low-mass protostars but the origins of the COM emission are still unclear. It can be associated with, for example, hot corinos, outflows, and/or accretion shock/disk atmosphere. We have conducte
Externí odkaz:
http://arxiv.org/abs/2403.16892
Autor:
Semenov, D., Henning, Th., Guilloteau, S., Smirnov-Pinchukov, G., Dutrey, A., Chapillon, E., Pietu, V., Franceschi, R., Schwarz, K., van Terwisga, S., Bouscasse, L., Caselli, P., Ceccarelli, C., Cunningham, N., Fuente, A., Gieser, C., Hsieh, T. -H., Lopez-Sepulcre, A., Segura-Cox, D. M., Pineda, J. E., Maureira, M. J., Moeller, Th., Tafalla, M., Valdivia-Mena, M. T.
Publikováno v:
A&A 685, A126 (2024)
We are performing a line survey of 8 planet-forming Class II disks in Taurus with the IRAM NOrthern Extended Millimeter Array (NOEMA), as a part of the MPG-IRAM Observatory Program PRODIGE (PROtostars and DIsks: Global Evolution; PIs: P. Caselli and
Externí odkaz:
http://arxiv.org/abs/2402.14653
Autor:
Hsieh, T. -H., Segura-Cox, D. M., Pineda, J. E., Caselli, P., Bouscasse, L., Neri, R., Lopez-Sepulcre, A., Valdivia-Mena, M. T., Maureira, M. J., Henning, Th., Smirnov-Pinchukov, G. V., Semenov, D., Möller, Th., Cunningham, N., Fuente, A., Marino, S., Dutrey, A., Tafalla, M., Chapillon, E., Ceccarelli, C., Zhao, B.
Publikováno v:
A&A 669, A137 (2023)
Aims. We present high sensitivity and high-spectral resolution NOEMA observations of the Class 0/I binary system SVS13A, composed of the low-mass protostars VLA4A and VLA4B with a separation of ~90 au. VLA4A is undergoing an accretion burst that enri
Externí odkaz:
http://arxiv.org/abs/2211.05022
Autor:
Meng, F., Sánchez-Monge, Á., Schilke, P., Padovani, M., Marcowith, A., Ginsburg, A., Schmiedeke, A., Schwörer, A., DePree, C., Veena, V. S., Möller, Th.
Publikováno v:
A&A 630, A73 (2019)
The giant molecular cloud Sagittarius B2 (hereafter SgrB2) is the most massive region with ongoing high-mass star formation in the Galaxy. In the southern region of the 40-pc large envelope of SgrB2, we encounter the SgrB2(DS) region which hosts more
Externí odkaz:
http://arxiv.org/abs/1908.07237
Publikováno v:
A&A 614, A123 (2018)
We model the emission of methyl cyanide (CH3CN) lines towards the massive hot molecular core SgrB2(M). We aim at reconstructing the CH3CN abundance field and investigating the gas temperature distribution as well as the velocity field. SgrB2(M) was o
Externí odkaz:
http://arxiv.org/abs/1802.09231
Autor:
Sanchez-Monge, A., Schilke, P., Schmiedeke, A., Ginsburg, A., Cesaroni, R., Lis, D. C., Qin, S. -L., Mueller, H. S. P., Bergin, E., Comito, C., Moeller, Th.
Publikováno v:
A&A 604, A6 (2017)
The high-mass star forming sites SgrB2(M) and SgrB2(N) have been the target of numerous studies, revealing e.g. a rich chemistry. We want to characterize their physical and chemical structure using ALMA high-angular resolution observations at mm wave
Externí odkaz:
http://arxiv.org/abs/1704.01805
Almost 200 different species have been detected in the interstellar medium (ISM) during the last decades, revealing not only simple species but complex molecules with more than 6 atoms. Other exotic compounds, like the weakly-bound dimer (H2)2, have
Externí odkaz:
http://arxiv.org/abs/1607.02749
Autor:
Schmiedeke, A., Schilke, P., Möller, Th., Sánchez-Monge, Á., Bergin, E., Comito, C., Csengeri, T., Lis, D. C., Molinari, S., Qin, S. -L., Rolffs, R.
Publikováno v:
A&A 588, A143 (2016)
We model the dust and free-free continuum emission in the high-mass star-forming region Sagittarius B2 in order to reconstruct the three-dimensional density and dust temperature distribution, as a crucial input to follow-up studies of the gas velocit
Externí odkaz:
http://arxiv.org/abs/1602.02274
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Akademický článek
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