The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point
Anthony P. Jones,Anthony P. Jones,L. Fanciullo,L. Fanciullo,M. Köhler,M. Köhler,L. Verstraete,L. Verstraete,Vincent Guillet,Vincent Guillet,M. Bocchio,M. Bocchio,Nathalie Ysard,Nathalie Ysard +13 more
TLDR
In this paper, a power-law distribution of small a-C grains and log-normal distributions of large a-SilFe and aC(:H) grains are used to explore dust evolution in the interstellar medium, and it is shown that mantle accretion in molecular clouds and UV photo-processing in photodominated regions are likely the major drivers of dust evolution.Abstract:
Context. The evolution of amorphous hydrocarbon materials, a-C(:H), principally resulting from ultraviolet (UV) photon absorption-induced processing, are likely at the heart of the variations in the observed properties of dust in the interstellar medium.Aims. The consequences of the size-dependent and compositional variations in a-C(:H), from aliphatic-rich a-C:H to aromatic-rich a-C, are studied within the context of the interstellar dust extinction and emission.Methods. Newly-derived optical property data for a-C(:H) materials, combined with that for an amorphous forsterite-type silicate with iron nano-particle inclusions, a-SilFe , are used to explore dust evolution in the interstellar medium.Results. We present a new dust model that consists of a power-law distribution of small a-C grains and log-normal distributions of large a-SilFe and a-C(:H) grains. The model, which is firmly anchored by laboratory-data, is shown to quite naturally explain the variations in the infrared (IR) to far-ultraviolet (FUV) extinction, the 217 nm UV bump, the IR absorption and emission bands and the IR-mm dust emission.Conclusions. The major strengths of the new model are its inherent simplicity and built-in capacity to follow dust evolution in interstellar media. We show that mantle accretion in molecular clouds and UV photo-processing in photo-dominated regions are likely the major drivers of dust evolution.read more
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Journal ArticleDOI
Planck 2018 results: XI. Polarized dust foregrounds
Yashar Akrami,Yashar Akrami,M. Ashdown,J. Aumont,Carlo Baccigalupi,Mario Ballardini,Mario Ballardini,A. J. Banday,A. J. Banday,R. B. Barreiro,Nicola Bartolo,Nicola Bartolo,Soumen Basak,K. Benabed,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,P. Bielewicz,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,F. Boulanger,F. Boulanger,F. Boulanger,Andrea Bracco,Andrea Bracco,M. Bucher,M. Bucher,Carlo Burigana,Carlo Burigana,Erminia Calabrese,Jean-François Cardoso,Julien Carron,H. C. Chiang,H. C. Chiang,C. Combet,B. P. Crill,P. de Bernardis,G. de Zotti,G. de Zotti,Jacques Delabrouille,J.-M. Delouis,E. Di Valentino,Clive Dickinson,Jose M. Diego,A. Ducout,X. Dupac,George Efstathiou,Franz Elsner,Torsten A. Enßlin,Edith Falgarone,Yabebal Fantaye,Yabebal Fantaye,Katia Ferrière,Katia Ferrière,Fabio Finelli,Francesco Forastieri,M. Frailis,A. A. Fraisse,E. Franceschi,Andrei V. Frolov,S. Galeotta,S. Galli,K. Ganga,Ricardo Genova-Santos,Ricardo Genova-Santos,Tuhin Ghosh,Tuhin Ghosh,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,Vincent Guillet,Vincent Guillet,Will Handley,F. K. Hansen,D. Herranz,Zhiqi Huang,Andrew H. Jaffe,W. C. Jones,E. Keihänen,Reijo Keskitalo,K. Kiiveri,K. Kiiveri,J. B. Kim,Nicoletta Krachmalnicoff,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,J.-M. Lamarre,Anthony Lasenby,M. Le Jeune,François Levrier,Michele Liguori,Michele Liguori,P. B. Lilje,V. Lindholm,V. Lindholm,M. López-Caniego,Philip Lubin,Yin-Zhe Ma,Yin-Zhe Ma,J. F. Macías-Pérez,Gianmarco Maggio,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,Peter G. Martin,E. Martínez-González,Sabino Matarrese,Sabino Matarrese,Jason D. McEwen,Peter Meinhold,Alessandro Melchiorri,M. Migliaccio,M. Migliaccio,M.-A. Miville-Deschênes,M.-A. Miville-Deschênes,Diego Molinari,Diego Molinari,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Paolo Natoli,Paolo Natoli,L. Pagano,L. Pagano,D. Paoletti,Valeria Pettorino,F. Piacentini,G. Polenta,J.-L. Puget,J.-L. Puget,Jörg P. Rachen,M. Reinecke,Mathieu Remazeilles,A. Renzi,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,B. Ruiz-Granados,B. Ruiz-Granados,L. Salvati,M. Sandri,M. Savelainen,M. Savelainen,M. Savelainen,Douglas Scott,Juan D. Soler,Locke D. Spencer,J. A. Tauber,D. Tavagnacco,D. Tavagnacco,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,Tiziana Trombetti,J. Valiviita,J. Valiviita,F. Vansyngel,B. Van Tent,P. Vielva,Fabrizio Villa,Nicola Vittorio,Ingunn Kathrine Wehus,Ingunn Kathrine Wehus,Andrea Zacchei,Andrea Zonca +183 more
TL;DR: In this paper, a power-law fit to the angular power spectra of dust polarization at 353 GHz for six nested sky regions covering from 24 to 71 % of the sky is presented.
Journal ArticleDOI
Planck intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
Peter A. R. Ade,M. I. R. Alves,G. Aniano,C. Armitage-Caplan,M. Arnaud,Fernando Atrio-Barandela,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,E. Battaner,Karim Benabed,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,P. Bielewicz,J. J. Bock,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,F. Boulanger,Carlo Burigana,Carlo Burigana,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,A. Chamballu,A. Chamballu,A. Chamballu,H. C. Chiang,H. C. Chiang,L. P. L. Colombo,L. P. L. Colombo,C. Combet,F. Couchot,A. Coulais,B. P. Crill,A. Curto,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,G. de Zotti,G. de Zotti,Jacques Delabrouille,F.-X. Désert,Clive Dickinson,Jose M. Diego,S. Donzelli,O. Doré,Marian Douspis,Joanna Dunkley,X. Dupac,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,Ken Ganga,Tuhin Ghosh,M. Giard,M. Giard,J. González-Nuevo,J. González-Nuevo,K. M. Górski,K. M. Górski,A. Gregorio,A. Gregorio,Alessandro Gruppuso,Vincent Guillet,F. K. Hansen,D. L. Harrison,George Helou,C. Hernández-Monteagudo,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,W. C. Jones,E. Keihänen,Reijo Keskitalo,Theodore Kisner,R. Kneissl,R. Kneissl,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,J.-M. Lamarre,Anthony Lasenby,Charles R. Lawrence,J. P. Leahy,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Antonio Mário Magalhães,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,N. Mandolesi,Michele Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,F. Noviello,Dmitry Novikov,I. D. Novikov,Niels Oppermann,Carol Anne Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,Fabio Pasian,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,L. Popa,G. W. Pratt,Jörg P. Rachen,Jörg P. Rachen,William T. Reach,Martin Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,Emanuele Salerno,M. Sandri,Giorgio Savini,Douglas Scott,Locke D. Spencer,V. Stolyarov,V. Stolyarov,Radek Stompor,Rashmikant V. Sudiwala,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,Matthieu Tristram,M. Tucci,M. Tucci,Luca Valenziano,Jussi Valiviita,B. Van Tent,P. Vielva,F. Villa,B. D. Wandelt,B. D. Wandelt,A. Zacchei,Andrea Zonca +226 more
TL;DR: In this paper, the authors use the Planck 353 GHz I, Q, and U Stokes maps as dust templates, and cross-correlate them with the planck and WMAP data at 12 frequencies from 23 to 353 GHz, over circular patches with 10° radius.
Journal ArticleDOI
The global dust modelling framework THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids)
TL;DR: The THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids) model as discussed by the authors is based upon a core model that was developed to explain the dust extinction and emission in the diffuse interstellar medium.
Journal ArticleDOI
The global dust modelling framework THEMIS
TL;DR: The THEMIS (The Heterogeneous dust Evolution Model for Interstellar Solids) model as discussed by the authors is based on a core model that was developed to explain the dust extinction and emission in the diffuse interstellar medium.
Journal ArticleDOI
Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies
Alain Abergel,Peter A. R. Ade,Nabila Aghanim,M. I. R. Alves,G. Aniano,Monique Arnaud,M. Ashdown,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,E. Battaner,K. Benabed,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,P. Bielewicz,Jérôme Bobin,Anna Bonaldi,J. R. Bond,François R. Bouchet,F. Boulanger,Carlo Burigana,Carlo Burigana,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,A. Chamballu,A. Chamballu,A. Chamballu,H. C. Chiang,H. C. Chiang,P. R. Christensen,David L. Clements,S. Colombi,L. P. L. Colombo,L. P. L. Colombo,F. Couchot,B. P. Crill,F. Cuttaia,Luigi Danese,R. J. Davis,P. de Bernardis,A. de Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,F.-X. Désert,Clive Dickinson,Jose M. Diego,H. Dole,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,E. Franceschi,S. Galeotta,K. Ganga,Tuhin Ghosh,M. Giard,M. Giard,Y. Giraud-Héraud,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,A. Gregorio,A. Gregorio,Alessandro Gruppuso,Vincent Guillet,F. K. Hansen,D. L. Harrison,George Helou,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,Gilles Joncas,Anthony P. Jones,W. C. Jones,Mika Juvela,P. M. W. Kalberla,E. Keihänen,J. Kerp,Reijo Keskitalo,Reijo Keskitalo,Theodore Kisner,R. Kneissl,R. Kneissl,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Anthony Lasenby,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,N. Mandolesi,M. Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Marcella Massardi,Sabino Matarrese,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,M. Migliaccio,Subhasish Mitra,Subhasish Mitra,M.-A. Miville-Deschênes,M.-A. Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,F. Noviello,Dmitry Novikov,I. D. Novikov,C. A. Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,F. Pasian,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,E. Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,N. Ponthieu,N. Ponthieu,L. Popa,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Jörg P. Rachen,William T. Reach,Rafael Rebolo,Rafael Rebolo,M. Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Ben Rusholme,M. Sandri,Giorgio Savini,Locke D. Spencer,Jean-Luc Starck,F. Sureau,D. Sutton,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,M. Tucci,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,B. Van Tent,Laurent Verstraete,P. Vielva,Fabrizio Villa,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Benjamin Winkel,D. Yvon,Andrea Zacchei,Andrea Zonca +248 more
TL;DR: In this article, the authors present a general methodology to study the dust-Hi correlation over the sky, including simulations to quantify uncertainties, and identify a Galactic contribution to these residuals with variations of the dust emissivity on angular scales smaller than that of their correlation analysis.
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