Zobrazeno 1 - 10
of 350
pro vyhledávání: '"I De Looze"'
Autor:
J. Rho, S.-H. Park, R. Arendt, M. Matsuura, D. Milisavljevic, T. Temim, I. De Looze, W. P. Blair, A. Rest, O. Fox, A. P. Ravi, B.-C. Koo, M. Barlow, A. Burrows, R. Chevalier, G. Clayton, R. Fesen, C. Fransson, C. Fryer, H. L. Gomez, H.-T. Janka, F. Kirchschlager, J. M. Laming, S. Orlando, D. Patnaude, G. Pavlov, P. Plucinsky, B. Posselt, F. Priestley, J. Raymond, N. Sartorio, F. Schmidt, P. Slane, N. Smith, N. Sravan, J. Vink, K. Weil, J. Wheeler, S. C. Yoon
Publikováno v:
The Astrophysical Journal Letters, Vol 969, Iss 1, p L9 (2024)
We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec Integral Field Unit (IFU) spectroscopy of the young Galactic supernova remnant Cassiopeia A (Cas A) to probe the physical conditions for molecular CO formation and d
Externí odkaz:
https://doaj.org/article/016bc259901442d3a49e82bfea30349c
Autor:
L Barrufet, P A Oesch, R Bouwens, H Inami, L Sommovigo, H Algera, E da Cunha, M Aravena, P Dayal, A Ferrara, Y Fudamoto, V Gonzalez, L Graziani, A P S Hygate, I de Looze, T Nanayakkara, A Pallottini, R Schneider, M Stefanon, M Topping, P van der Werf
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522(3):3926-3934
We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a ultraviolet (UV)-selected galaxy sample with the Atacama Large Millimeter Array (ALMA) spectroscopic observations. Our an
Autor:
Maria Niculescu-Duvaz, M J Barlow, William Dunn, Antonia Bevan, Omar Ahmed, David Arkless, Jon Barker, Sidney Bartolotta, Liam Brockway, Daniel Browne, Ubaid Esmail, Max Garner, Wiktoria Guz, Scarlett King, Hayri Kose, Madeline Lampstaes-Capes, Joseph Magen, Nicole Morrison, Kyaw Oo, Balvinder Paik, Joanne Primrose, Danny Quick, Anais Radeka, Anthony Rodney, Eleanor Sandeman, Fawad Sheikh, Camron Stansfield, Delayne Symister, Joshua Taylor, William Wilshere, R Wesson, I De Looze, G C Clayton, K Krafton, M Matsuura
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:2940-2950
Core-collapse supernovae (CCSNe) are potentially capable of producing large quantities of dust, with strong evidence that ejecta dust masses can grow significantly over extended periods of time. Red-blue asymmetries in the broad emission lines of CCS
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Shockwaves driven by supernovae both destroy dust and reprocess the surviving grains, greatly affecting the resulting dust properties of the interstellar medium (ISM). While these processes have been extensively studied theoretically, observational c
Autor:
A P S Hygate, J A Hodge, E da Cunha, M Rybak, S Schouws, H Inami, M Stefanon, L Graziani, R Schneider, P Dayal, R J Bouwens, R Smit, R A A Bowler, R Endsley, V Gonzalez, P A Oesch, D P Stark, H S B Algera, M Aravena, L Barrufet, A Ferrara, Y Fudamoto, J H A Hilhorst, I De Looze, T Nanayakkara, A Pallottini, D A Riechers, L Sommovigo, M W Topping, P van der Werf
We present Atacama Large Millimeter/Submillimeter Array (ALMA) [CII] and $\sim158$ $\rm\mu m$ continuum observations of REBELS-25, a massive, morphologically complex ultra-luminous infrared galaxy (ULIRG; $L_{\rm IR}=1.5^{+0.8}_{-0.5}\times10^{12}$ L
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6218f2d3be90e76d1f169ef55b122dcf
https://hdl.handle.net/11384/132062
https://hdl.handle.net/11384/132062
Akademický článek
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Akademický článek
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Akademický článek
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Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
The ratio of the mass of interstellar dust to the total mass of metals (the dust-to-metals/DTM ratio) tends to increase with metallicity. This can be explained by the increasing efficiency of grain growth in the interstellar medium (ISM) at higher me
Autor:
Maria Niculescu-Duvaz, M J Barlow, A Bevan, R Wesson, D Milisavljevic, I De Looze, G C Clayton, K Krafton, M Matsuura, R Brady
Publikováno v:
Monthly Notices of the Royal Astronomical Society
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Modelling the red-blue asymmetries seen in the broad emission lines of core-collapse supernovae (CCSNe) is a powerful technique to quantify total dust mass formed in the ejecta at late times ($>5$ years after outburst) when ejecta dust temperatures b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec7930019b461ece6e31f667b17acb94
https://orca.cardiff.ac.uk/id/eprint/152108/1/stac1626.pdf
https://orca.cardiff.ac.uk/id/eprint/152108/1/stac1626.pdf