Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Rico-Villas F"'
Using high angular resolution ALMA observations ($0.02^{\prime\prime}\approx0.34$ pc), we study the thermal structure and kinematics of the proto super star cluster $13$ in the central region of NGC253 through their continuum and vibrationally excite
Externí odkaz:
http://arxiv.org/abs/2208.01941
Autor:
Colzi, L., Martín-Pintado, J., Rivilla, V. M., Jiménez-Serra, I., Zeng, S., Rodríguez-Almeida, L. F., Rico-Villas, F., Martín, S., Requena-Torres, M. A.
The Central Molecular Zone (CMZ) contains most of the mass of our Galaxy but its star formation rate is one order of magnitude lower than in the Galactic disc. This is likely related to the fact that the bulk of the gas in the CMZ is in a warm ($>$10
Externí odkaz:
http://arxiv.org/abs/2202.04111
Autor:
Cosentino, G., Jiménez-Serra, I., Tan, J. C., Henshaw, J. D., Barnes, A. T., Law, C. -Y., Zeng, S., Fontani, F., Caselli, P., Viti, S., Zahorecz, S., Rico-Villas, F., Megías, A., Miceli, M., Orlando, S., Ustamujic, S., Greco, E., Peres, G., Bocchino, F., Fedriani, R., Gorai, P., Testi, L., Martín-Pintado, J.
Supernova remnants (SNRs) contribute to regulate the star formation efficiency and evolution of galaxies. As they expand into the interstellar medium (ISM), they transfer vast amounts of energy and momentum that displace, compress and heat the surrou
Externí odkaz:
http://arxiv.org/abs/2201.03008
Autor:
Almeida, L. F. Rodríguez, Rivilla, V. M., Jiménez-Serra, I., Melosso, M., Colzi, L., Zeng, S., Tercero, B., de Vicente, P., Martín, S., Requena-Torres, M. A., Rico-Villas, F., Martín-Pintado, J.
Publikováno v:
A&A 654, L1 (2021)
Little is known about the chemistry of isocyanates (compounds with the functional group R-N=C=O) in the interstellar medium, as only four of them have been detected so far: isocyanate radical (NCO), isocyanic acid (HNCO), N-protonated isocyanic acid
Externí odkaz:
http://arxiv.org/abs/2109.07889
Autor:
Rivilla, V. M., Jiménez-Serra, I., de la Concepción, J. García, Martín-Pintado, J., Colzi, L., Rodríguez-Almeida, L. F., Tercero, B., Rico-Villas, F., Zeng, S., Martín, S., Requena-Torres, M. A., de Vicente, P.
We report here the first detection in the interstellar medium of the cyanomidyl radical (HNCN). Using the Yebes 40m and the IRAM 30m telescopes, we have targeted the doublets of the $N$=2$-$1, 4$-$3, 5$-$4, 6$-$5, and 7$-$6 transitions of HNCN toward
Externí odkaz:
http://arxiv.org/abs/2106.09652
Autor:
Martín, S., Martín-Pintado, J., Blanco-Sánchez, C., Rivilla, V. M., Rodríguez-Franco, A., Rico-Villas, F.
Publikováno v:
A&A 631, A159 (2019)
In this paper we present the detailed formalism at the core of the Spectral Line Identification and Modelling (SLIM) within the MAdrid Data CUBe Analysis (MADCUBA) package and their main data handling functionalities. These tools have been developed
Externí odkaz:
http://arxiv.org/abs/1909.02147
Autor:
González-Alfonso, E., Armus, L., Carrera, F. J., Charmandaris, V., Efstathiou, A., Egami, E., Fernández-Ontiveros, J. A., Fischer, J., Granato, G. L., Gruppioni, C., Hatziminaoglou, E., Imanishi, M., Isobe, N., Kaneda, H., Koziel-Wierzbowska, D., Malkan, M. A., Martin-Pintado, J., Mateos, S., Matsuhara, H., Miniutti, G., Nakagawa, T., Pozzi, F., Rico-Villas, F., Rodighiero, G., Roelfsema, P., Spinoglio, L., Spoon, H. W. W., Sturm, E., van der Tak, F., Vignali, C., Wang, L.
A far-infrared observatory such as the {\it SPace Infrared telescope for Cosmology and Astrophysics} ({\it SPICA}), with its unprecedented spectroscopic sensitivity, would unveil the role of feedback in galaxy evolution during the last $\sim10$ Gyr o
Externí odkaz:
http://arxiv.org/abs/1710.02356
Autor:
Kajava, J. J. E., Rico-Villas, F.
Nearby galaxies host ultra-luminous X-ray sources (ULXs), whose nature remains largely unknown. Until the discovery of the first ULX pulsar, M82 X-2, the mechanism powering the large luminosities of most ULXs was thought to be super-Eddington accreti
Externí odkaz:
http://arxiv.org/abs/1609.03941
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