Zobrazeno 1 - 10
of 64
pro vyhledávání: '"Clark, C.J.R."'
Autor:
Katsioli S., Adam R., Ade P., Ajeddig H., André P., Artis E., Aussel H., Baes M., Beelen A., Benoît A., Berta S., Bing L., Bourrion O., Calvo M., Catalano A., Clark C.J.R., De Looze I., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Ejlali G., Galametz M., Galliano F., Gomez A., Goupy J., Hanser C., Hughes A., Kéruzoré F., Kramer C., Jones A.P., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Madden S.C., Maury A., Mauskopf P., Mayet F., Monfardini A., Moyer-Anin A., Muñoz-Echeverría M., Nersesian A., Pantoni L., Paradis D., Perotto L., Pisano G., Ponthieu N., Revéret V., Rigby A.J., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Sievers A., Smith M.W.L., Tedros J., Tabatabaei F., Tucker C., Xilouris E.M., Ysard N., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 293, p 00026 (2024)
In the framework of the IMEGIN Large Program, we used the NIKA2 camera on the IRAM 30-m telescope to observe the edge-on galaxy NGC 891 at 1.15 mm and 2 mm and at a FWHM of 11.1” and 17.6”, respectively. Multiwavelength data enriched with the new
Externí odkaz:
https://doaj.org/article/dbcd72540bd04dbf9e6052d6adaf688f
Akademický článek
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Aims. The purpose of this work is the characterization of the main scaling relations between all of the interstellar medium (ISM) components, namely dust, atomic, molecular, and total gas, and gas-phase metallicity, as well as other galaxy properties
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::88669bbe03cb7b4c7e0111c64df627a3
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068812
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068812
Context. Dust in late-type galaxies in the local Universe is responsible for absorbing approximately one third of the energy emitted by stars. It is often assumed that dust heating is mainly attributable to the absorption of ultraviolet and optical p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::f115d9e910065b5e093cb173ebb8996a
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068729
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068729
Context. Interstellar dust absorbs stellar light very efficiently, thus shaping the energy output of galaxies. Studying the impact of different stellar populations on the dust heating continues to be a challenge because it requires decoupling the rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::94b0e64903c1362a7151c4b75c3eb6bb
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068741
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068741
Context. Dust plays an important role in shaping a galaxy's spectral energy distribution (SED). It absorbs ultraviolet (UV) to near-infrared radiation and re-emits this energy in the far-infrared (FIR). The FIR is essential to understand dust in gala
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::e9a5b008d18da3d39f3c29a8e3d4a92c
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068782
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068782
Aims. Within the framework of the DustPedia project we investigate the properties of cosmic dust and its interaction with stellar radiation (originating from di erent stellar populations) for 814 galaxies in the nearby Universe, all observed by the H
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::8ac7f594abe805975274ed2032c2f318
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068987
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068987
Aims. We compare the far-infrared to sub-millimetre dust emission properties measured in high Galactic latitude cirrus with those determined in a sample of 204 late-type DustPedia galaxies. The aim is to verify if it is appropriate to use Milky Way d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::2e62e262899963167efc661f54363782
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068871
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068871
Most radiative transfer models assume that dust in spiral galaxies is distributed exponentially. In this paper our goal is to verify this assumption by analysing the two-dimensional large-scale distribution of dust in galaxies from the DustPedia samp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::aa443fec5c0102917bc271502f5cfb13
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069040
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069040
Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to-gas ratios in a sub-sample of ~500 DustPedia galaxies. Using literat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::1f38f84d523684a0afb21606f2ae584d
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069015
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069015