| Naslov: | THE RISE OF SN 2014J IN THE NEARBY GALAXY M82 |
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| Avtorji: | ID Goobar, Ariel, The Oskar Klein Centre, Physics Department, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden (Avtor)
ID Johansson, Joel, The Oskar Klein Centre, Physics Department, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden (Avtor)
ID Amanullah, Rahman, The Oskar Klein Centre, Physics Department, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden (Avtor)
ID Cao, Yi, Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA (Avtor)
ID Kasliwal, Mansi, Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA (Avtor)
ID Ferretti, Raphael, The Oskar Klein Centre, Physics Department, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden (Avtor)
ID Nugent, Peter, 4 Computational Cosmology Center, Computational Research Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50B-4206, Berkeley, CA 94720, USA 5 Department of Astronomy, University of California Berkeley, B-20 Hearst Field Annex # 3 (Avtor)
ID Perley, Daniel, Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA (Avtor)
ID Gal-Yam, Avishay, Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel (Avtor)
ID Ofek, Eran, Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100, Israel (Avtor)
ID Tendulkar, S. P., Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA (Avtor)
ID Dennefeld, M., CNRS, Institut d’Astrophysique de Paris (IAP) and University P. et M. Curie (Paris 6), 98bis Boulevard Arago, F-75014 Paris, France 8 (Avtor)
ID Valenti, Stefano, Las Cumbres Observatory Global Telescope Network, 6740 Corona Drive, Suite 102, Goleta, CA 93117, USA 9 Department of Physics, University of California, Santa Barbara, Broida Hall, Mail Code 9530, Santa Barbara, CA 93106-9530, USA (Avtor)
ID Arcavi, Iair, Las Cumbres Observatory Global Telescope Network, 6740 Corona Drive, Suite 102, Goleta, CA 93117, USA (Avtor)
ID Banerjee, D.P.K., Physical Research Laboratory, Ahmedabad 380 009, India (Avtor)
ID Venkataraman, V., Physical Research Laboratory, Ahmedabad 380 009, India (Avtor)
ID Cenko, Brad, Astrophysics Science Division, NASA Goddard Space Flight Center, Mail Code 661, Greenbelt, MD 20771, USA 13 Joint Space Science Institute, University of Maryland, College Park, MD 20742, USA (Avtor)
ID Petrushevska, Tanja, The Oskar Klein Centre, Physics Department, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden (Avtor)
ID Dupuy, T.J., Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA (Avtor)
ID Liu, M.C., Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA (Avtor), et al. |
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| Datoteke: |
Gradivo nima datotek, ki so prostodostopne za javnost. Gradivo je morda fizično dosegljivo v knjižnici fakultete, zalogo lahko preverite v COBISS-u.  |
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| Jezik: | Angleški jezik |
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| Vrsta gradiva: | Delo ni kategorizirano |
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| Tipologija: | 1.01 - Izvirni znanstveni članek |
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| Organizacija: | UNG - Univerza v Novi Gorici
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| Opis: | We report on the discovery of SN 2014J in the nearby galaxy M82. Given its proximity, it offers the best opportunity
to date to study a thermonuclear supernova (SN) over a wide range of the electromagnetic spectrum. Optical, nearIR,
and mid-IR observations on the rising light curve, orchestrated by the intermediate Palomar Transient Factory,
show that SN 2014J is a spectroscopically normal Type Ia supernova (SN Ia), albeit exhibiting high-velocity features
in its spectrum and heavily reddened by dust in the host galaxy. Our earliest detections start just hours after the
fitted time of explosion. We use high-resolution optical spectroscopy to analyze the dense intervening material and
do not detect any evolution in the resolved absorption features during the light curve rise. Similar to other highly
reddened SNe Ia, a low value of total-to-selective extinction, RV 2, provides the best match to our observations.
We also study pre-explosion optical and near-IR images from Hubble Space Telescope with special emphasis on
the sources nearest to the SN location. |
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| Ključne besede: | dust, extinction – galaxies: individual (Messier 82) – supernovae: individual (SN 2014J) |
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| Verzija publikacije: | Objavljena publikacija |
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| Leto izida: | 2014 |
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| Št. strani: | 6 |
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| Številčenje: | 784, L12 |
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| PID: | 20.500.12556/RUNG-3562-ca2fc2cc-98fe-29fe-e91d-35929dd6f6d0 |
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| COBISS.SI-ID: | 4995835 |
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| DOI: | 10.1088/2041-8205/784/1/L12 |
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| NUK URN: | URN:SI:UNG:REP:FLJK7APB |
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| Datum objave v RUNG: | 22.01.2018 |
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| Število ogledov: | 4833 |
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| Število prenosov: | 0 |
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| Metapodatki: |    |
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