Zobrazeno 1 - 10
of 746
pro vyhledávání: '"Finger R."'
Autor:
Mena, F. P., Valenzuela, D., Espinoza, C., Pizarro, F., Tan, B. -K., Thoen, D. J., Baselmans, J. J. A., Finger, R.
Achieving amplification with high gain and quantum-limited noise is a difficult problem to solve. Parametric amplification using a superconducting transmission line with high kinetic inductance is a promising technology not only to solve this problem
Externí odkaz:
http://arxiv.org/abs/2310.15344
Publikováno v:
A&A 677, A148 (2023)
(Abridged) High-mass star formation is far less understood than low-mass star formation. It entails molecular outflows, which disturb the protostellar clump. Studying these outflows and the shocked gas they cause is key for a better understanding of
Externí odkaz:
http://arxiv.org/abs/2307.16350
Autor:
Gallardo, D.1 (AUTHOR) diego.gallardo@raig.uchile.cl, Finger, R.1,2 (AUTHOR), Solis, F.1 (AUTHOR), Monasterio, D.3 (AUTHOR), Jorquera, S.2 (AUTHOR), Pizarro, J.1 (AUTHOR), Riquelme, J.1 (AUTHOR), Curotto, F.1 (AUTHOR), Pizarro, F.4 (AUTHOR), Bronfman, L.1 (AUTHOR)
Publikováno v:
Journal of Astronomical Instrumentation. Jun2024, Vol. 13 Issue 2, p1-16. 16p.
Autor:
Duronea, N. U., Cichowolski, S., Bronfman, L., Mendoza, E., Finger, R., Suad, L. A., Corti, M., Reynoso, E. M.
Publikováno v:
A&A 646, A103 (2021)
With the aim of studying the properties of Galactic IR bubbles and their impact in massive star formation, we present a study of the IR bubble S169, associated with the massive star forming region IRAS12326-6245. We used CO(2-1),$^{13}$CO(2-1), C$^{1
Externí odkaz:
http://arxiv.org/abs/2012.06328
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:
Duronea, N. U., Bronfman, L., Mendoza, E., Merello, M., Finger, R., Reyes, N., Hervías-Caimapo, C., Faure, A., Cappa, C. E., Arnal, E. M., Lépine, J. R. D., Kleiner, I., Nyman, L-Ä
Using APEX-1 and APEX-2 observations, we have detected and studied the rotational lines of the HC$_3$N molecule (cyanoacetylene) in the powerful outflow/hot molecular core G331.512-0.103. We identified thirty-one rotational lines at $J$ levels betwee
Externí odkaz:
http://arxiv.org/abs/1907.09479
Akademický článek
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Autor:
Rodriguez, R., Finger, R., Mena, F. P., Alvear, A., Fuentes, R., Khudchenko, A., Hesper, R., Baryshev, A. M., Reyes, N., Bronfman, L.
Publikováno v:
A&A 619, A153 (2018)
In observational radio astronomy, sideband-separating receivers are preferred, particularly under high atmospheric noise, which is usually the case in the sub-millimeter range. However, obtaining a good rejection ratio between the two sidebands is di
Externí odkaz:
http://arxiv.org/abs/1806.04053
Autor:
Nguyen, Hiep, Dawson, J. R., Miville-Deschênes, M. -A., Tang, Ningyu, Li, Di, Heiles, Carl, Murray, Claire E., Stanimirović, Snežana, Gibson, Steven J., McClure-Griffiths, N. M., Troland, Thomas, Bronfman, L., Finger, R.
Observations of interstellar dust are often used as a proxy for total gas column density $N_\mathrm{H}$. By comparing $\textit{Planck}$ thermal dust data (Release 1.2) and new dust reddening maps from Pan-STARRS 1 and 2MASS (Green et al. 2018), with
Externí odkaz:
http://arxiv.org/abs/1805.11787