Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae

M Arnaud; F Atrio-Barandela; J Aumont; C Baccigalupi; AJ Banday; RB Barreiro; E Battaner; K Benabed; A Benoit-Lévy; JP Bernard; M Bersanelli; P Bielewicz; A Bonaldi; JR Bond; J Borrill; FR Bouchet; CS Buemi; C Burigana; JF Cardoso; S Casassus; A Catalano; L Cerrigone; A Chamballu; HC Chiang; S Colombi; LPL Colombo; F Couchot; BP Crill; A Curto; F Cuttaia; RD Davies; RJ Davis; P De Bernardis; A De Rosa; G De Zotti; J Delabrouille; C Dickinson; JM Diego; S Donzelli; O Doré; X Dupac; TA Enßlin; HK Eriksen; F Finelli; M Frailis; E Franceschi; S Galeotta; K Ganga; M Giard; J González-Nuevo; KM Górski; A Gregorio; A Gruppuso; FK Hansen; DL Harrison; SR Hildebrandt; E Hivon; WA Holmes; JL Hora; A Hornstrup; W Hovest; KM Huffenberger; TR Jaffe; WC Jones; M Juvela; E Keihänen; R Keskitalo; TS Kisner; J Knoche; M Kunz; H Kurki-Suonio; A Lähteenmäki; JM Lamarre; A Lasenby; CR Lawrence; R Leonardi; P Leto; PB Lilje; M Linden-Vørnle; M López-Caniego; JF Macías-Pérez; B Maffei; D Maino; N Mandolesi; PG Martin; S Masi; M Massardi; S Matarrese; P Mazzotta; L Mendes; A Mennella; M Migliaccio; MA Miville-Deschênes; A Moneti; L Montier; G Morgante; D Mortlock; D Munshi; JA Murphy; P Naselsky

Journal article

Planck intermediate results XVIII the millimetre and sub-millimetre emission from planetary nebulae

M Arnaud, F Atrio-Barandela, J Aumont, C Baccigalupi, AJ Banday, RB Barreiro, E Battaner, K Benabed, A Benoit-Lévy, JP Bernard, M Bersanelli, P Bielewicz, A Bonaldi, JR Bond, J Borrill, FR Bouchet, CS Buemi, C Burigana, JF Cardoso, S Casassus Show all

Astronomy and Astrophysics | EDP SCIENCES S A | Published : 2015

DOI: 10.1051/0004-6361/201423836

Abstract

Late stages of stellar evolution are characterized by copious mass-loss events whose signature is the formation of circumstellar envelopes (CSE). Planck multi-frequency measurements have provided relevant information on a sample of Galactic planetary nebulae (PNe) in the important and relatively unexplored observational band between 30 and 857 GHz. Planck enables the assembly of comprehensive PNe spectral energy distributions (SEDs) from radio to far-IR frequencies. Modelling the derived SEDs provides us with information on physical properties of CSEs and the mass content of both main components: ionized gas, traced by the free-free emission at cm-mm waves; and thermal dust, traced by the mi..

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University of Melbourne Researchers

Pietro Procopio Author

Grants

Awarded by National Aeronautics and Space Administration

Funding Acknowledgements

The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planck&page=Planck_Collaboration The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. L. Cerrigone acknowledges funding from the Spanish Consejo Superior de Investigaciones Cientificas through a JAE-Doc research contract, co-funded by the European Social Fund. L. C. thanks the Spanish MICINN for funding support through grants AYA2009-07304 and CSD2009-00038.