Zobrazeno 1 - 10
of 990
pro vyhledávání: '"Falgarone , E."'
Autor:
Kim, W. -J., Schilke, P., Neufeld, D. A., Jacob, A. M., Sánchez-Monge, Á., Seifried, D., Godard, B., Menten, K. M., Walch, S., Falgarone, E., Veena, V. S., Bialy, S., Möller, T., Wyrowski, F.
Publikováno v:
A&A 670, A111 (2023)
As a complement to the HyGAL Stratospheric Observatory for Infrared Astronomy Legacy Program, we report the results of a ground-based absorption line survey of simple molecules in diffuse and translucent Galactic clouds. Using the Institut de Radioas
Externí odkaz:
http://arxiv.org/abs/2212.09334
Autor:
Appleton, P. N., Emonts, B., Lisenfeld, U., Falgarone, E., Guillard, P., Boulanger, F., Braine, J., Ogle, P., Struck, C., Vollmer, B., Yeager, T.
We present ALMA observations at a spatial resolution of 0.2 arcsec (60 pc) of CO emission from the Taffy galaxies (UGC 12914/5). The observations are compared with narrow-band Pa$\alpha$, mid-IR, radio continuum and X-ray imaging, plus optical spectr
Externí odkaz:
http://arxiv.org/abs/2203.17142
Autor:
Jacob, A. M., Neufeld, D. A., Schilke, P., Wiesemeyer, H., Kim, W., Bialy, S., Busch, M., Elia, D., Falgarone, E., Gerin, M., Godard, B., Higgins, R., Hennebelle, P., Indriolo, N., Lis, D. C., Menten, K. M., Sanchez-Monge, A., Ossenkopf-Okada, V., Rugel, M. R., Seifried, D., Sonnentrucker, P., Walch, S., Wolfire, M., Wyrowski, F., Valdivia, V.
The HyGAL SOFIA legacy program surveys six hydride molecules -- ArH+, OH+, H2O+, SH, OH, and CH -- and two atomic constituents -- C+ and O -- within the diffuse interstellar medium (ISM) by means of absorption-line spectroscopy toward 25 bright Galac
Externí odkaz:
http://arxiv.org/abs/2202.05046
Autor:
Vidal-García, A., Falgarone, E., Battaia, F. Arrigoni, Godard, B., Ivison, R. J., Zwaan, M. A., Herrera, C., Frayer, D., Andreani, P., Li, Q., Gavazzi, R.
We present a comparative analysis of the $\rm CH^+$(1-0) and $\rm Ly \alpha$ lines, observed with the Atacama Large Millimeter Array (ALMA) and Keck telescope respectively, in the field of the submillimetre-selected galaxy (SMG) SMM\,J02399$-$0136 at
Externí odkaz:
http://arxiv.org/abs/2105.10202
Autor:
Paladini, R., Mottram, J. C., Veneziani, M., Traficante, A., Schisano, E., Giardino, G., Falgarone, E., Urquhart, J. S., Harrison, D. L., Joncas, G., Umana, G., Molinari, S.
Massive star formation occurs in the interior of giant molecular clouds (GMC) and proceeds through many stages. In this work, we focus on massive young stellar objects (MYSOs) and Ultra-Compact HII regions (UCHII), where the former are enshrouded in
Externí odkaz:
http://arxiv.org/abs/2102.08494
Autor:
Guillard, P., Appleton, P. N, Boulanger, F., Shull, J. M., Lehnert, M. D., Forets, G. Pineau des, Falgarone, E., Cluver, M. E., Xu, C. K., Gallagher, S. C., Duc, P. A.
We present Hubble Space Telescope Cosmic Origin Spectrograph (COS) UV line spectroscopy and integral-field unit (IFU) observations of the intra-group medium in Stephan's Quintet (SQ). SQ hosts a 30 kpc long shocked ridge triggered by a galaxy collisi
Externí odkaz:
http://arxiv.org/abs/2102.06843
Publikováno v:
A&A 643, A101 (2020)
Shocks are ubiquitous in the interstellar and intergalactic media, where their chemical and radiative signatures reveal the physical conditions in which they arise. Detailed astrochemical models of shocks at all velocities are necessary to understand
Externí odkaz:
http://arxiv.org/abs/2010.01042
Publikováno v:
A&A 641, A124 (2020)
(abridged) We present ALMA observations of hydrogen fluoride, HF J=1-0, H20 (220-211), and the 1.2 THz rest-frame continuum emission from the z=4.7 system BR1202-0725. BR1202-0725 is a galaxy group consisting of a QSO, a sub-millimeter galaxy (SMG),
Externí odkaz:
http://arxiv.org/abs/2004.04176
Autor:
Ivison, R. J., Richard, J., Biggs, A. D., Zwaan, M. A., Falgarone, E., Arumugam, V., van der Werf, P. P., Rujopakarn, W.
With the spatial resolution of the Atacama Large Millimetre Array (ALMA), dusty galaxies in the distant Universe typically appear as single, compact blobs of dust emission, with a median half-light radius, $\approx$ 1 kpc. Occasionally, strong gravit
Externí odkaz:
http://arxiv.org/abs/2003.07863
Autor:
André, Ph., Hughes, A., Guillet, V., Boulanger, F., Bracco, A., Ntormousi, E., Arzoumanian, D., Maury, A. J., Bernard, J. -Ph., Bontemps, S., Ristorcelli, I., Girart, J. M., Motte, F., Tassis, K., Pantin, E., Montmerle, T., Johnstone, D., Gabici, S., Efstathiou, A., Basu, Shantanu, Béthermin, M., Beuther, H., Braine, J., Di Francesco, J., Falgarone, E., Ferrière, K., Fletcher, A., Galametz, M., Giard, M., Hennebelle, P., Jones, A., Kepley, A. A., Kwon, J., Lagache, G., Lesaffre, P., Levrier, F., Li, D., Li, Z. -Y., Mao, S. A., Nakagawa, T., Onaka, T., Paladino, R., Peretto, N., Poglitsch, A., Revéret, V., Rodriguez, L., Sauvage, M., Soler, J. D., Spinoglio, L., Tabatabaei, F., Tritsis, A., van der Tak, F., Ward-Thompson, D., Wiesemeyer, H., Ysard, N., Zhang, H.
Publikováno v:
PASA, 36, e029 (2019)
SPICA, the cryogenic infrared space telescope recently pre-selected for a `Phase A' concept study as one of the three remaining candidates for ESA's fifth medium class (M5) mission, is foreseen to include a far-infrared polarimetric imager (SPICA-POL
Externí odkaz:
http://arxiv.org/abs/1905.03520