Zobrazeno 1 - 10
of 108
pro vyhledávání: '"Wienen, M."'
Autor:
Neralwar, K. R., Colombo, D., Duarte-Cabral, A., Urquhart, J. S., Mattern, M., Wyrowski, F., Menten, K. M., Barnes, P., Sanchez-Monge, A., Rigby, A. J., Mazumdar, P., Eden, D., Csengeri, T., Dobbs, C. L., Veena, V. S., Neupane, S., Henning, T., Schuller, F., Leurini, S., Wienen, M., Yang, A. Y., Ragan, S. E., Medina, S., Nguyen-Luong, Q.
Publikováno v:
A&A 664, A84 (2022)
The Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium (SEDIGISM) survey has produced high (spatial and spectral) resolution $^{13}$CO (2-1) maps of the Milky Way. It has allowed us to investigate the molecular interstellar
Externí odkaz:
http://arxiv.org/abs/2205.02253
Autor:
Neralwar, K. R., Colombo, D., Duarte-Cabral, A., Urquhart, J. S., Mattern, M., Wyrowski, F., Menten, K. M., Barnes, P., Sanchez-Monge, A., Beuther, H., Rigby, A. J., Mazumdar, P., Eden, D., Csengeri, T., Dobbs, C. L., Veena, V. S., Neupane, S., Henning, T., Schuller, F., Leurini, S., Wienen, M., Yang, A. Y., Ragan, S. E., Medina, S., Nguyen-Luong, Q.
Publikováno v:
A&A 663, A56 (2022)
We present one of the very first extensive classifications of a large sample of molecular clouds based on their morphology. This is achieved using a recently published catalogue of 10663 clouds obtained from the first data release of the SEDIGISM sur
Externí odkaz:
http://arxiv.org/abs/2203.02504
Autor:
Colombo, D., König, C., Urquhart, J. S., Wyrowski, F., Mattern, M., Menten, K. M., Lee, M. -Y., Brand, J., Wienen, M., Mazumdar, P., Schuller, F., Leurini, S.
Publikováno v:
A&A 655, L2 (2021)
Filaments are a ubiquitous morphological feature of the molecular interstellar medium and are identified as sites of star formation. In recent years, more than 100 large-scale filaments (with a length $>10$\,pc) have been observed in the inner Milky
Externí odkaz:
http://arxiv.org/abs/2111.02768
Autor:
Colombo, D., Duarte-Cabral, A., Pettitt, A. R., Urquhart, J. S., Wyrowski, F., Csengeri, T., Neralwar, K. R., Schuller, F., Menten, K. M., Anderson, L., Barnes, P., Beuther, H., Bronfman, L., Eden, D., Ginsburg, A., Henning, T., Koenig, C., Lee, M. -Y., Mattern, M., Medina, S., Ragan, S. E., Rigby, A. J., Sanchez-Monge, A., Traficante, A., Yang, A. Y., Wienen, M.
Publikováno v:
A&A 658, A54 (2022)
The morphology of the Milky Way is still a matter of debate. In order to shed light on uncertainties surrounding the structure of the Galaxy, in this paper, we study the imprint of spiral arms on the distribution and properties of its molecular gas.
Externí odkaz:
http://arxiv.org/abs/2110.06071
Autor:
Wienen, M., Wyrowski, F., Walmsley, C. M., Csengeri, T., Pillai, T., Giannetti, A., Menten, K. M.
Publikováno v:
A&A 649, A21 (2021)
Deuteration has been used as a tracer of the evolutionary phases of low- and high-mass star formation. The APEX Telescope Large Area Survey (ATLASGAL) provides an important repository for a detailed statistical study of massive star-forming clumps in
Externí odkaz:
http://arxiv.org/abs/2102.04478
Autor:
Schuller, F., Urquhart, J. S., Csengeri, T., Colombo, D., Duarte-Cabral, A., Mattern, M., Ginsburg, A., Pettitt, A. R., Wyrowski, F., Anderson, L., Azagra, F., Barnes, P., Beltran, M., Beuther, H., Billington, S., Bronfman, L., Cesaroni, R., Dobbs, C., Eden, D., Lee, M. -Y., Medina, S. -N. X., Menten, K. M., Moore, T., Montenegro-Montes, F. M., Ragan, S., Rigby, A., Riener, M., Russeil, D., Schisano, E., Sanchez-Monge, A., Traficante, A., Zavagno, A., Agurto, C., Bontemps, S., Finger, R., Giannetti, A., Gonzalez, E., Hernandez, A. K., Henning, T., Kainulainen, J., Kauffmann, J., Leurini, S., Lopez, S., Mac-Auliffe, F., Mazumdar, P., Molinari, S., Motte, F., Muller, E., Nguyen-Luong, Q., Parra, R., Perez-Beaupuits, J. -P., Schilke, P., Schneider, N., Suri, S., Testi, L., Torstensson, K., Veena, V. S., Venegas, P., Wang, K., Wienen, M.
The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg^2 of the Galactic plane between l = -60 deg and l = +31 deg in several molecular transitions, including 13CO(2-1)
Externí odkaz:
http://arxiv.org/abs/2012.01527
Autor:
Duarte-Cabral, A., Colombo, D., Urquhart, J. S., Ginsburg, A., Russeil, D., Schuller, F., Anderson, L. D., Barnes, P. J., Beltran, M. T., Beuther, H., Bontemps, S., Bronfman, L., Csengeri, T., Dobbs, C. L., Eden, D., Giannetti, A., Kauffmann, J., Mattern, M., Medina, S. -N. X., Menten, K. M., Lee, M. -Y., Pettitt, A. R., Riener, M., Rigby, A. J., Trafficante, A., Veena, V. S., Wienen, M., Wyrowski, F., Agurto, C., Azagra, F., Cesaroni, R., Finger, R., Gonzalez, E., Henning, T., Hernandez, A. K., Kainulainen, J., Leurini, S., Lopez, S., Mac-Auliffe, F., Mazumdar, P., Molinari, S., Motte, F., Muller, E., Nguyen-Luong, Q., Parra, R., Perez-Beaupuits, J. -P., Montenegro-Montes, F. M., Moore, T. J. T., Ragan, S. E., Sanchez-Monge, A., Sanna, A., Schilke, P., Schisano, E., Schneider, N., Suri, S., Testi, L., Torstensson, K., Venegas, P., Wang, K., Zavagno, A.
We use the 13CO(2-1) emission from the SEDIGISM high-resolution spectral-line survey of the inner Galaxy, to extract the molecular cloud population with a large dynamic range in spatial scales, using the SCIMES algorithm. This work compiles a cloud c
Externí odkaz:
http://arxiv.org/abs/2012.01502
Autor:
Urquhart, J. S., Figura, C., Cross, J. R., Wells, M. R. A., Moore, T. J. T., Eden, D. J., Ragan, S. E., Pettitt, A. R., Duarte-Cabral, A., Colombo, D., Schuller, F., Csengeri, T., Mattern, M., Beuther, H., Menten, K. M., Wyrowski, F., Anderson, L. D., Barnes, P. J., Beltrán, M. T., Billington, S. J., Bronfman, L., Giannetti, A., Kainulainen, J., Kauffmann, J., Lee, M. -Y., Leurini, S., Medina, S. -N. X., Montenegro-Montes, F. M., Riener, M., Rigby, A. J., Sánchez-Monge, A., Schilke, P., Schisano, E., Traficante, A., Wienen, M.
By combining two surveys covering a large fraction of the molecular material in the Galactic disk we investigate the role the spiral arms play in the star formation process. We have matched clumps identified by ATLASGAL with their parental GMCs as id
Externí odkaz:
http://arxiv.org/abs/2012.01464
Autor:
Sabatini, G., Bovino, S., Giannetti, A., Wyrowski, F., Órdenes, M. A., Pascale, R., Pillai, T., Wienen, M., Csengeri, T., Menten, K. M.
Publikováno v:
A&A 644, A34 (2020)
(Abridged) We present a large sample of o-H$_2$D$^+$ observations in high-mass star-forming regions and discuss possible empirical correlations with relevant physical quantities to assess its role as a chronometer of star-forming regions through diff
Externí odkaz:
http://arxiv.org/abs/2009.12108
Autor:
Barnes, A. T., Kauffmann, J., Bigiel, F., Brinkmann, N., Colombo, D., Guzmán, A. E, Kim, W. J., Szűcs, L., Wakelam, V., Aalto, S., Albertsson, T., Evans II, N. J., Glover, S. C. O., Goldsmith, P. F., Kramer, C., Menten, K., Nishimura, Y., Viti, S., Watanabe, Y., Weiss, A., Wienen, M., Wiesemeyer, H., Wyrowski, F.
The current generation of (sub)mm-telescopes has allowed molecular line emission to become a major tool for studying the physical, kinematic, and chemical properties of extragalactic systems, yet exploiting these observations requires a detailed unde
Externí odkaz:
http://arxiv.org/abs/2007.11005