Zobrazeno 1 - 10
of 636
pro vyhledávání: '"Jones, B. M."'
Autor:
Avison, A., Fuller, G. A., Frimpong, N. Asabre, Etoka, S., Hoare, M., Jones, B. M., Peretto, N., Traficante, A., van der Tak, F., Pineda, J. E., Beltrán, M., Wyrowski, F., Thompson, M., Lumsden, S., Nagy, Z., Hill, T., Viti, S., Fontani, F., Schilke, P.
The role of massive ($\geq$ 8M$_{\odot}$) stars in defining the energy budget and chemical enrichment of the interstellar medium in their host galaxy is significant. In this first paper from the Tracing Evolution in Massive Protostellar Objects (TEMP
Externí odkaz:
http://arxiv.org/abs/2309.05772
Autor:
Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J., Beelen, A., Weiss, A., Nanni, A., Omont, A., van der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C.
Publikováno v:
A&A 678, A28 (2023)
The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM NOrthern Extended Millimeter Array, with the aim to measure their redshift and study their properties. Several of them have been resolved into multiple sources. Consequently
Externí odkaz:
http://arxiv.org/abs/2307.15748
Autor:
Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-Fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C.
Publikováno v:
A&A 678, A26 (2023)
(Abridged) Using the IRAM NOEMA interferometer, we measures the redshifts of 126 bright galaxies detected in the Herschel H-ATLAS, HeLMS, and HerS surveys. We report reliable spectroscopic redshifts for a total of 124 of the Herschel-selected galaxie
Externí odkaz:
http://arxiv.org/abs/2307.15732
Autor:
Stanley, F., Jones, B. M., Riechers, D. A., Yang, C., Berta, S., Cox, P., Bakx, T. J. L. C., Cooray, A., Dannerbauer, H., Dye, S., Hughes, D. H., Ivison, R. J., Jin, S., Lehnert, M., Neri, R., Omont, A., van der Werf, P., Weiss, A.
We present the results of a survey of CO(1-0) emission in 14 infrared luminous dusty star forming galaxies (DSFGs) at 2 < z < 4 with the NSF's Karl G. Jansky Very Large Array. All sources are detected in CO(1-0), with an ~1arcsec angular resolution.
Externí odkaz:
http://arxiv.org/abs/2301.12976
Autor:
Traficante, A., Jones, B. M., Avison, A., Fuller, G. A., Benedettini, M., Elia, D., Molinari, S., Peretto, N., Pezzuto, S., Pillai, T., Rygl, K. L. J., Schisano, E., Smith, R. J.
The formation mechanism of the most massive stars is far from completely understood. It is still unclear if the formation is core-fed or clump-fed, i.e. if the process is an extension of what happens in low-mass stars, or if the process is more dynam
Externí odkaz:
http://arxiv.org/abs/2301.09917
Autor:
Bendo, G. J., Urquhart, S. A., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M. D., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., González-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Jones, B. M., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Pérez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., van der Werf, P., Verma, A., Vlahakis, C., Weiß, A., Yang, C., Young, A. J.
We present 101 and 151 GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500 micron flux densities >80 mJy and 250-500 micron colours consistent with z > 2, most of which are expected to be gravitationally lensed o
Externí odkaz:
http://arxiv.org/abs/2301.02584
Autor:
Berta, S., Young, A. J., Cox, P., Neri, R., Jones, B. M., Baker, A. J., Omont, A., Dunne, L., Rosell, A. Carnero, Marchetti, L., Negrello, M., Yang, C., Riechers, D. A., Dannerbauer, H., Perez-Fournon, I., van der Werf, P., Bakx, T., Ivison, R. J., Beelen, A., Buat, V., Cooray, A., Cortzen, I., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Jin, S., Krips, M., Lagache, G., Lehnert, M., Messias, H., Serjeant, S., Stanley, F., Urquhart, S., Vlahakis, C., Weiss, A.
Publikováno v:
A&A 646, A122 (2021)
(Abridged) Exploiting the sensitivity and broad band width of NOEMA, we have studied the molecular gas and dust in the galaxy HerBS-89a, at z=2.95. High angular resolution images reveal a partial 1.0" diameter Einstein ring in the dust continuum emis
Externí odkaz:
http://arxiv.org/abs/2012.01448
Autor:
Jones, B. M., Fuller, G. A., Breen, S. L., Avison, A., Green, J. A., Traficante, A., Elia, D., Ellingsen, S. P., Voronkov, M. A., Merello, M., Molinari, S., Schisano, E.
The Methanol MultiBeam survey (MMB) provides the most complete sample of Galactic massive young stellar objects (MYSOs) hosting 6.7GHz class II methanol masers. We characterise the properties of these maser sources using dust emission detected by the
Externí odkaz:
http://arxiv.org/abs/2001.08449
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Akademický článek
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