Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Montes, A. M."'
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:
Solarz, A., Thomas, R., Montenegro-Montes, F. M., Gromadzki, M., Donoso, E., Koprowski, M., Wyrzykowski, L., Diaz, C. G., Sani, E., Bilicki, M.
Publikováno v:
A&A 642, A103 (2020)
We present the results of a programme to search and identify the nature of unusual sources within the All-sky Wide-field Infrared Survey Explorer (WISE) that is based on a machine-learning algorithm for anomaly detection, namely one-class support vec
Externí odkaz:
http://arxiv.org/abs/2008.10658
Autor:
Montes-Solís, M., Arregui, I.
We use Coronal Multi-channel Polarimeter (CoMP) observations of propagating waves in the solar corona and Bayesian analysis to assess the evidence of models with resonant damping and foot-point wave power asymmetries. Two nested models are considered
Externí odkaz:
http://arxiv.org/abs/2008.03004
Publikováno v:
A&A 625, A35 (2019)
A classic application of coronal seismology uses transverse oscillations of waveguides to obtain estimates of the magnetic field strength. The procedure requires information on the density of the structures. Often, it ignores the damping of the oscil
Externí odkaz:
http://arxiv.org/abs/1903.05437
Autor:
Montes-Solís, M., Arregui, I.
Publikováno v:
A&A 622, A88 (2019)
High resolution observations have permitted to resolve the solar prominences/filaments as sets of threads/fibrils. However, the values of the physical parameters of these threads and their structuring remain poorly constrained. We use prominence seis
Externí odkaz:
http://arxiv.org/abs/1812.07262
Autor:
Belitsky, V., Lapkin, I., Fredrixon, M., Meledin, D., Sundin, E., Billade, B., Ferm, S. -E., Pavolotsky, A., Rashid, H., Strandberg, M., Desmaris, V., Ermakov, A., Krause, S., Olberg, M., Aghdam, P., Shafiee, S., Bergman, P., De Beck, E., Olofsson, H., Conway, J., De Breuck, C., Immer, K., Yagoubov, P., Montenegro-Montes, F. M., Torstensson, K., Pérez-Beaupuits, J. -P., Klein, T., Boland, W., Baryshev, A. M., Hesper, R., Barkhof, J., Adema, J., Bekema, M. E., Koops, A.
Context: We describe the new SEPIA (Swedish-ESO PI Instrument for APEX) receiver, which was designed and built by the Group for Advanced Receiver Development (GARD), at Onsala Space Observatory (OSO) in collaboration with ESO. It was installed and co
Externí odkaz:
http://arxiv.org/abs/1712.07396
Autor:
Montes-Solís, M., Arregui, I.
Publikováno v:
The Astrophysical Journal, 2017, Volume 846, Number 2
We present a method to assess the plausibility of alternative mechanisms to explain the damping of magnetohydrodynamic (MHD) transverse waves in solar coronal loops. The considered mechanisms are resonant absorption of kink waves in the Alfv\'en cont
Externí odkaz:
http://arxiv.org/abs/1709.03347
Autor:
Schuller, F., Csengeri, T., Urquhart, J. S., Duarte-Cabral, A., Barnes, P. J., Giannetti, A., Hernandez, A. K., Leurini, S., Mattern, M., Medina, S. -N. X., Agurto, C., Azagra, F., Anderson, L. D., Beltrán, M. T., Beuther, H., Bontemps, S., Bronfman, L., Dobbs, C. L., Dumke, M., Finger, R., Ginsburg, A., Gonzalez, E., Henning, T., Kauffmann, J., Mac-Auliffe, F., Menten, K. M., Montenegro-Montes, F. M., Moore, T. J. T., Muller, E., Parra, R., Perez-Beaupuits, J. -P., Pettitt, A., Russeil, D., Sánchez-Monge, Á., Schilke, P., Schisano, E., Suri, S., Testi, L., Torstensson, K., Venegas, P., Wang, K., Wienen, M., Wyrowski, F., Zavagno, A.
Publikováno v:
A&A 601, A124 (2017)
The origin and life-cycle of molecular clouds are still poorly constrained, despite their importance for understanding the evolution of the interstellar medium. We have carried out a systematic, homogeneous, spectroscopic survey of the inner Galactic
Externí odkaz:
http://arxiv.org/abs/1701.04712