Zobrazeno 1 - 10
of 123
pro vyhledávání: '"Mininni C"'
Autor:
Wells, M. R. A., Beuther, H., Molinari, S., Schilke, P., Battersby, C., Ho, P., Sánchez-Monge, Á., Jones, B., Scheuck, M. B., Syed, J., Gieser, C., Kuiper, R., Elia, D., Coletta, A., Traficante, A., Wallace, J., Rigby, A. J., Klessen, R. S., Zhang, Q., Walch, S., Beltrán, M. T., Tang, Y., Fuller, G. A., Lis, D. C., Möller, T., van der Tak, F., Klaassen, P. D., Clarke, S. D., Moscadelli, L., Mininni, C., Zinnecker, H., Maruccia, Y., Pezzuto, S., Benedettini, M., Soler, J. D., Brogan, C. L., Avison, A., Sanhueza, P., Schisano, E., Liu, T., Fontani, F., Rygl, K. L. J., Wyrowski, F., Bally, J., Walker, D. L., Ahmadi, A., Koch, P., Merello, M., Law, C. Y., Testi, L.
Publikováno v:
A&A 690, A185 (2024)
We use data from the ALMA Evolutionary Study of High Mass Protocluster Formation in the Galaxy (ALMAGAL) survey to study 100 ALMAGAL regions at $\sim$ 1 arsecond resolution located between $\sim$ 2 and 6 kpc distance. Using ALMAGAL $\sim$ 1.3mm line
Externí odkaz:
http://arxiv.org/abs/2408.08299
Autor:
López-Gallifa, Á., Rivilla, V. M., Beltrán, M. T., Colzi, L., Mininni, C., Sánchez-Monge, Á., Fontani, F., Viti, S., Jiménez-Serra, I., Testi, L., Cesaroni, R., Lorenzani, A.
Most stars, including the Sun, are born in rich stellar clusters containing massive stars. Therefore, the study of the chemical reservoir of massive star-forming regions is crucial to understand the basic chemical ingredients available at the dawn of
Externí odkaz:
http://arxiv.org/abs/2403.02191
Autor:
Fontani, F., Mininni, C., Beltrán, M. T., Rivilla, V. M., Colzi, L., Jiménez-Serra, I., López-Gallifa, Á., Sánchez-Monge, Á., Viti, S.
The astrochemistry of the important biogenic element phosphorus (P) is still poorly understood, but observational evidence indicates that P-bearing molecules are likely associated with shocks. We study P-bearing molecules, as well as some shock trace
Externí odkaz:
http://arxiv.org/abs/2311.13367
Autor:
Soler, J. D., Zari, E., Elia, D., Molinari, S., Mininni, C., Schisano, E., Traficante, A., Klessen, R. S., Glover, S. C. O., Hennebelle, P., Colman, T., Frankel, N., Wenger, T.
Publikováno v:
A&A 678, A95 (2023)
We present a comparison of the Milky Way's star formation rate (SFR) surface density ($\Sigma_{\rm SFR}$) obtained with two independent state-of-the-art observational methods. The first method infers $\Sigma_{\rm SFR}$ from observations of the dust t
Externí odkaz:
http://arxiv.org/abs/2308.01330
Autor:
Mininni, C., Beltrán, M. T., Colzi, L., Rivilla, V. M., Fontani, F., Lorenzani, A., López-Gallifa, Á., Viti, S., Sánchez-Monge, Á., Schilke, P., Testi, L.
The G31.41+0.31 Unbiased ALMA sPectral Observational Survey (GUAPOS) project targets the hot molecular core (HMC) G31.41+0.31 (G31), to unveil the complex chemistry of one of the most chemically rich high-mass star-forming regions outside the Galacti
Externí odkaz:
http://arxiv.org/abs/2306.13563
Autor:
Soler, J. D., Zucker, C., Peek, J. E. G., Heyer, M., Goldsmith, P. F., Glover, S. C. O., Molinari, S., Klessen, R. S., Hennebelle, P., Testi, L., Colman, T., Benedettini, M., Elia, D., Mininni, C., Pezzuto, S., Schisano, E., Traficante, A.
Publikováno v:
A&A 675, A206 (2023)
We present a study of the three-dimensional (3D) distribution of interstellar dust derived from stellar extinction observations toward the Taurus molecular cloud (MC) and its relation with the neutral atomic hydrogen (HI) emission at 21 cm wavelength
Externí odkaz:
http://arxiv.org/abs/2305.13180
Autor:
Elia, D., Molinari, S., Schisano, E., Soler, J. D., Merello, M., Russeil, D., Veneziani, M., Zavagno, A., Noriega-Crespo, A., Olmi, L., Benedettini, M., Hennebelle, P., Klessen, R. S., Leurini, S., Paladini, R., Pezzuto, S., Traficante, A., Eden, D. J., Martin, P. G., Sormani, M., Coletta, A., Colman, T., Plume, R., Maruccia, Y., Mininni, C., Liu, S. J.
We present a new derivation of the Milky Way's current star formation rate (SFR) based on the data of the Hi-GAL Galactic plane survey. We estimate the distribution of the SFR across the Galactic plane from the star-forming clumps identified in the H
Externí odkaz:
http://arxiv.org/abs/2211.05573
Autor:
de la Concepción, J. García, Colzi, L., Jiménez-Serra, I., Molpeceres, G., Corchado, J. C., Rivilla, V. M., Martín-Pintado, J., Beltrán, M. T., Mininni, C.
We studied theoretically the cis-trans isomerization reactions of two astrophysically relevant acids, formic acid (HCOOH) and thioformic acid (HC(O)SH), where the latter has recently been discovered in space. We also searched for these molecules towa
Externí odkaz:
http://arxiv.org/abs/2111.10842
Autor:
Colzi, L., Rivilla, V. M., Beltrán, M. T., Jiménez-Serra, I., Mininni, C., Melosso, M., Cesaroni, R., Fontani, F., Lorenzani, A., Sánchez-Monge, A., Viti, S., Schilke, P., Testi, L., Alonso, E. R., Kolesniková, L.
Publikováno v:
A&A 653, A129 (2021)
Peptide-like bond molecules, which can take part to the formation of proteins in a primitive Earth environment, have been detected up to now only towards a few sources. We present a study of HNCO, HC(O)NH$_{2}$, CH$_{3}$NCO, CH$_{3}$C(O)NH$_{2}$, CH$
Externí odkaz:
http://arxiv.org/abs/2107.11258
Autor:
Mininni, C., Fontani, F., Sánchez-Monge, A., Rivilla, V. M., Beltrán, M. T., Zahorecz, S., Immer, K., Giannetti, A., Caselli, P., Colzi, L., Testi, L., Elia, D.
Publikováno v:
A&A 653, A87 (2021)
The TOPG\"ot project studies a sample of 86 high-mass star-forming regions in different evolutionary stages from starless cores to ultra compact HII regions. The aim of the survey is to analyze different molecular species in a statistically significa
Externí odkaz:
http://arxiv.org/abs/2107.10741