IAS/CEA Evolution of Dust in Nearby Galaxies (ICED): the spatially-resolved dust properties of NGC4254

• Published in: arXiv.org
• Main Authors: Pantoni, L, 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, De Petris, M, Désert, F -X, Doyle, S, Driessen, E F C, Ejlali, G, Galliano, F, Gomez, A, Goupy, J, Jones, A P, Hanser, C, Hughes, A, Katsioli, S, Kéruzoré, F, Kramer, C, Ladjelate, B, Lagache, G, Leclercq, S, J -F Lestrade, Macías-Pérez, J F, Madden, S C, Maury, A, Mauskopf, P, Mayet, F, Monfardini, A, Moyer-Anin, A, Muñoz-Echeverría, M, Nersesian, A, 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, M W S L Smith, Tabatabaei, F S, Tedros, J, Tucker, C, Xilouris, E M, Zylka, R
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 10.10.2023
• Subjects: Correlation; Cosmic dust; Dust; Galaxies; Interstellar matter; Interstellar radiation; Line spectra; Metallicity; Parameters; Physics - Astrophysics of Galaxies; Radiation; Spectral energy distribution; Star formation; Sublimation; Vapor phases
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2310.06463

We present the first preliminary results of the project \textit{ICED}, focusing on the face-on galaxy NGC4254. We use the millimetre maps observed with NIKA2 at IRAM-30m, as part of the IMEGIN Guaranteed Time Large Program, and of a wide collection of ancillary data (multi-wavelength photometry and gas phase spectral lines) that are publicly available. We derive the global and local properties of interstellar dust grains through infrared-to-radio spectral energy distribution fitting, using the hierarchical Bayesian code HerBIE, which includes the grain properties of the state-of-the-art dust model, THEMIS. Our method allows us to get the following dust parameters: dust mass, average interstellar radiation field, and fraction of small grains. Also, it is effective in retrieving the intrinsic correlations between dust parameters and interstellar medium properties. We find an evident anti-correlation between the interstellar radiation field and the fraction of small grains in the centre of NGC4254, meaning that, at strong radiation field intensities, very small amorphous carbon grains are efficiently destroyed by the ultra-violet photons coming from newly formed stars, through photo-desorption and sublimation. We observe a flattening of the anti-correlation at larger radial distances, which may be driven by the steep metallicity gradient measured in NGC4254.