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Naslov:THE PECULIAR EXTINCTION LAW OF SN 2014J MEASURED WITH THE HUBBLE SPACE TELESCOPE
Avtorji:ID Amanullah, Rahman, Oskar Klein Centre, Physics Department, Stockholm University, SE-106 91 Stockholm, Sweden (Avtor)
ID Goobar, Ariel, Oskar Klein Centre, Physics Department, Stockholm University, SE-106 91 Stockholm, Sweden (Avtor)
ID Johansson, Joel, Oskar Klein Centre, Physics Department, Stockholm University, SE-106 91 Stockholm, Sweden (Avtor)
ID Banerjee, D.P.K., Physical Research Laboratory, Ahmedabad 380009, India (Avtor)
ID Venkataraman, V., Physical Research Laboratory, Ahmedabad 380009, India (Avtor)
ID Joshi, V., Physical Research Laboratory, Ahmedabad 380009, India (Avtor)
ID Ashok, N.M., Physical Research Laboratory, Ahmedabad 380009, India (Avtor)
ID Cao, Yi, Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA (Avtor)
ID Kasliwal, Mansi, Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101, USA (Avtor)
ID Kulkarni, S.R., Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA (Avtor)
ID Nugent, P.E., Department of Astronomy, University of California Berkeley, B-20 Hearst Field, Annex # 3411, Berkeley, CA 94720-3411, USA 6 Computational Cosmology Center, Computational Research Division, Lawrence Berkeley National Laboratory, (Avtor)
ID Petrushevska, Tanja, Oskar Klein Centre, Physics Department, Stockholm University, SE-106 91 Stockholm, Sweden (Avtor)
ID Stanishev, V., CENTRA—Centro Multidisciplinar de Astrof´ısica, Instituto Superior Tecnico, Av. Rovisco Pais 1, 1049-001 Lisbon, Portugal (Avtor), et al.
Datoteke: Gradivo nima datotek, ki so prostodostopne za javnost. Gradivo je morda fizično dosegljivo v knjižnici fakultete, zalogo lahko preverite v COBISS-u. Povezava se odpre v novem oknu
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:UNG - Univerza v Novi Gorici
Opis:The wavelength dependence of the extinction of Type Ia SN 2014J in the nearby galaxy M82 has been measured using UV to near-IR photometry obtained with the Hubble Space Telescope, the Nordic Optical Telescope, and the Mount Abu Infrared Telescope. This is the first time that the reddening of an SN Ia is characterized over the full wavelength range of 0.2–2μm. A total-to-selective extinction, RV 3.1, is ruled out with high significance. The best fit at maximum using a Galactic type extinction law yields RV = 1.4 ± 0.1. The observed reddening of SN 2014J is also compatible with a power-law extinction, Aλ/AV = (λ/λV ) p as expected from multiple scattering of light, with p = −2.1 ± 0.1. After correcting for differences in reddening, SN 2014J appears to be very similar to SN 2011fe over the 14 broadband filter light curves used in our study.
Ključne besede:dust, extinction – galaxies: individual (Messier 82) – supernovae: individual SN2014J
Verzija publikacije:Objavljena publikacija
Leto izida:2014
Št. strani:6
Številčenje:788, L21
PID:20.500.12556/RUNG-3564-53f49ed8-5695-4bb9-6995-d4d36857aba5 Novo okno
COBISS.SI-ID:4996347 Novo okno
DOI:10.1088/2041-8205/788/2/L21 Novo okno
NUK URN:URN:SI:UNG:REP:T62J1WRD
Datum objave v RUNG:22.01.2018
Število ogledov:4167
Število prenosov:0
Metapodatki:XML DC-XML DC-RDF
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Naslov:Astrophysical Journal Letters
Skrajšan naslov:APJL
Založnik:American Astronomical Society
Leto izida:2014
ISSN:2041-8205

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