Zobrazeno 1 - 10
of 367
pro vyhledávání: '"G. A. Fuller"'
Autor:
T Irabor, M G Hoare, M Burton, W D Cotton, P Diamond, S Dougherty, S P Ellingsen, R Fender, G A Fuller, S Garrington, P F Goldsmith, J Green, A G Gunn, J Jackson, S Kurtz, S L Lumsden, J Marti, I McDonald, S Molinari, T J Moore, M Mutale, T Muxlow, T O’Brien, R D Oudmaijer, R Paladini, J D Pandian, J M Paredes, A M S Richards, A Sanchez-Monge, R Spencer, M A Thompson, G Umana, J S Urquhart, M Wieringa, A Zijlstra
We present the first high spatial resolution radio continuum survey of the southern Galactic plane. The CORNISH project has mapped the region defined by 295° < l < 350°; |b| < 1° at 5.5 GHz, with a resolution of 2.5 arcsec (FWHM). As with the CORN
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38c57152c2125492cc9b088426d46347
https://resolver.caltech.edu/CaltechAUTHORS:20230321-821389800.58
https://resolver.caltech.edu/CaltechAUTHORS:20230321-821389800.58
Autor:
A Traficante, B M Jones, A Avison, G A Fuller, M Benedettini, D Elia, S Molinari, N Peretto, S Pezzuto, T Pillai, K L J Rygl, E Schisano, R J Smith
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:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc68713a46a69fc48f5bc63933341764
http://arxiv.org/abs/2301.09917
http://arxiv.org/abs/2301.09917
Publikováno v:
Atmospheric Chemistry and Physics, Vol 15, Iss 17, Pp 10107-10125 (2015)
Positive matrix factorisation (PMF) analysis was applied to PM10 chemical composition and particle number size distribution (NSD) data measured at an urban background site (North Kensington) in London, UK, for the whole of 2011 and 2012. The PMF anal
Externí odkaz:
https://doaj.org/article/393c99b5d4d54697a9a19eb410ed97ff
Particulate matter from wood burning emissions (Cwood) was quantified at five locations in the United Kingdom (UK), comprising three rural and two urban sites between 2009 and 2021. The aethalometer method was used. Mean winter Cwood concentrations r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::201a1477c52efbb20bb8a004025dce15
http://hdl.handle.net/10044/1/100066
http://hdl.handle.net/10044/1/100066
Autor:
P. Nazari, J. D. Meijerhof, M. L. van Gelder, A. Ahmadi, E. F. van Dishoeck, B. Tabone, D. Langeroodi, N. F. W. Ligterink, J. Jaspers, M. T. Beltrán, G. A. Fuller, Á. Sánchez-Monge, P. Schilke
Publikováno v:
Astronomy & Astrophysics, 668:A109
Nazari, P, Meijerhof, J D, van Gelder, M L, Ahmadi, A, van Dishoeck, E F, Tabone, B, Langeroodi, D, Ligterink, N F W, Jaspers, J, Beltran, M T, Fuller, G A, Sanchez-Monge, A & Schilke, P 2022, ' N-bearing complex organics toward high-mass protostars Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range ', Astronomy & Astrophysics, vol. 668, A109 . https://doi.org/10.1051/0004-6361/202243788
Nazari, P, Meijerhof, J D, van Gelder, M L, Ahmadi, A, van Dishoeck, E F, Tabone, B, Langeroodi, D, Ligterink, N F W, Jaspers, J, Beltran, M T, Fuller, G A, Sanchez-Monge, A & Schilke, P 2022, ' N-bearing complex organics toward high-mass protostars Constant ratios pointing to formation in similar pre-stellar conditions across a large mass range ', Astronomy & Astrophysics, vol. 668, A109 . https://doi.org/10.1051/0004-6361/202243788
No statistical study of COMs toward a large sample of high-mass protostars with ALMA has been carried out so far. We aim to study six N-bearing species: CH$_3$CN, HNCO, NH$_2$CHO, C$_2$H$_5$CN, C$_2$H$_3$CN and CH$_3$NH$_2$ in a large sample of high-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9450eff579ea8feb970cab39b05ed151
Autor:
M. L. van Gelder, J. Jaspers, P. Nazari, A. Ahmadi, E. F. van Dishoeck, M. T. Beltrán, G. A. Fuller, Á. Sánchez-Monge, P. Schilke
Publikováno v:
Astronomy & Astrophysics, 667:A136
The deuteration of molecules forming in the ices such as methanol (CH$_3$OH) is sensitive to the physical conditions during their formation in dense cold clouds and can be probed through observations of deuterated methanol in hot cores. Observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf32a197af88ab0e80f1340e3b23d936
https://ui.adsabs.harvard.edu/abs/2022A&A...667A.136V
https://ui.adsabs.harvard.edu/abs/2022A&A...667A.136V
Autor:
M. L. van Gelder, P. Nazari, B. Tabone, A. Ahmadi, E. F. van Dishoeck, M. T. Beltrán, G. A. Fuller, N. Sakai, Á. Sánchez-Monge, P. Schilke, Y.-L. Yang, Y. Zhang
Publikováno v:
Astronomy & Astrophysics, 662:A67
Complex organic molecules (COMs) are often observed toward embedded Class 0 and I protostars. However, not all Class 0 and I protostars exhibit COMs emission. In this work, variations in methanol (CH$_3$OH) emission are studied to test if absence of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ba37ceffd0ee3fbd8e4c3e40f1167a8
https://hdl.handle.net/1887/3515475
https://hdl.handle.net/1887/3515475
Publikováno v:
Astronomy & Astrophysics
Autor:
S. Martín, J. G. Mangum, N. Harada, F. Costagliola, K. Sakamoto, S. Muller, R. Aladro, K. Tanaka, Y. Yoshimura, K. Nakanishi, R. Herrero-Illana, S. Mühle, S. Aalto, E. Behrens, L. Colzi, K. L. Emig, G. A. Fuller, S. García-Burillo, T. R. Greve, C. Henkel, J. Holdship, P. Humire, L. Hunt, T. Izumi, K. Kohno, S. König, D. S. Meier, T. Nakajima, Y. Nishimura, M. Padovani, V. M. Rivilla, S. Takano, P. P. van der Werf, S. Viti, Y. T. Yan
Publikováno v:
Martín, S, Mangum, J G, Harada, N, Costagliola, F, Sakamoto, K, Muller, S, Aladro, R, Tanaka, K, Yoshimura, Y, Nakanishi, K, Herrero-Illana, R, Mühle, S, Aalto, S, Behrens, E, Colzi, L, Emig, K L, Fuller, G A, García-Burillo, S, Greve, T R, Henkel, C, Holdship, J, Humire, P, Hunt, L, Izumi, T, Kohno, K, König, S, Meier, D S, Nakajima, T, Nishimura, Y, Padovani, M, Rivilla, V M, Takano, S, Van Der Werf, P P, Viti, S & Yan, Y T 2021, ' ALCHEMI, an AL MA Comprehensive High-resolution Extragalactic Molecular Inventory : Survey presentation and first results from the ACA array ', Astronomy and Astrophysics, vol. 656, A46 . https://doi.org/10.1051/0004-6361/202141567
Martin, S, Mangum, J G, Harada, N, Costagliola, F, Sakamoto, K, Muller, S, Aladro, R, Tanaka, K, Yoshimura, Y, Nakanishi, K, Herrero-Illana, R, Muehle, S, Aalto, S, Behrens, E, Colzi, L, Emig, K L, Fuller, G A, Garcia-Burillo, S, Greve, T R, Henkel, C, Holdship, J, Humire, P, Hunt, L, Izumi, T, Kohno, K, Koenig, S, Meier, D S, Nakajima, T, Nishimura, Y, Padovani, M, Rivilla, V M, Takano, S, van der Werf, P P, Viti, S & Yan, Y T 2021, ' ALCHEMI, an ALMA Comprehensive High-resolution Extragalactic Molecular Inventory Survey presentation and first results from the ACA array ', Astronomy & Astrophysics, vol. 656, A46 . https://doi.org/10.1051/0004-6361/202141567
Astronomy & Astrophysics, 656
Digital.CSIC. Repositorio Institucional del CSIC
instname
Martin, S, Mangum, J G, Harada, N, Costagliola, F, Sakamoto, K, Muller, S, Aladro, R, Tanaka, K, Yoshimura, Y, Nakanishi, K, Herrero-Illana, R, Muehle, S, Aalto, S, Behrens, E, Colzi, L, Emig, K L, Fuller, G A, Garcia-Burillo, S, Greve, T R, Henkel, C, Holdship, J, Humire, P, Hunt, L, Izumi, T, Kohno, K, Koenig, S, Meier, D S, Nakajima, T, Nishimura, Y, Padovani, M, Rivilla, V M, Takano, S, van der Werf, P P, Viti, S & Yan, Y T 2021, ' ALCHEMI, an ALMA Comprehensive High-resolution Extragalactic Molecular Inventory Survey presentation and first results from the ACA array ', Astronomy & Astrophysics, vol. 656, A46 . https://doi.org/10.1051/0004-6361/202141567
Astronomy & Astrophysics, 656
Digital.CSIC. Repositorio Institucional del CSIC
instname
Martín, S., et al.
[Context] The interstellar medium is the locus of physical processes affecting the evolution of galaxies which drive or are the result of star formation activity, supermassive black hole growth, and feedback. The resulting ph
[Context] The interstellar medium is the locus of physical processes affecting the evolution of galaxies which drive or are the result of star formation activity, supermassive black hole growth, and feedback. The resulting ph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f93ca0c0ffb102abb1a137e69043614
https://orbit.dtu.dk/en/publications/d8d619a7-4a8f-4458-90f5-96250a79c7ed
https://orbit.dtu.dk/en/publications/d8d619a7-4a8f-4458-90f5-96250a79c7ed
Autor:
Matt Golding, Alastair K. H. MacGibbon, G. Thomas Fuller, Thérèse Considine, Lara Matia-Merino
Publikováno v:
Food Biophysics. 13:80-90
We investigated the effects of Tween emulsifier fatty acid chain length on the shear stability and crystallization behavior of 35 wt% partially crystalline oil-in-water emulsions prepared with and without 1 wt% sodium caseinate. Emulsions containing