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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
earth and planetary sciences
Panchromatic observations of SN2011dh point to a compact progenitor star
Astrophysical Journal, Volume 752, No. 2, Article 78, Year 2012
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Description
We report the discovery and detailed monitoring of X-ray emission associated with the TypeIIbSN2011dh using data from the Swift and Chandra satellites, placing it among the best-studied X-ray supernovae (SNe) to date. We further present millimeter and radio data obtained with the Submillimeter Array, the Combined Array for Research in Millimeter-wave Astronomy, and the Expanded Very Large Array during the first three weeks after explosion. Combining these observations with early optical photometry, we show that the panchromatic data set is well described by non-thermal synchrotron emission (radio/mm) with inverse Compton scattering (X-ray) of a thermal population of optical photons. In this scenario, the shock partition fractions deviate from equipartition by a factor, (εe/εB) 30. We derive the properties of the shock wave and the circumstellar environment and find a time-averaged shock velocity of and a progenitor mass-loss rate of (for an assumed wind velocity, vw = 1000 km s-1). We show that these properties are consistent with the sub-class of TypeIIbSNe characterized by compact progenitors (TypecIIb) and dissimilar from those with extended progenitors (Type eIIb). Furthermore, we consider the early optical emission in the context of a cooling envelope model to estimate a progenitor radius of R * 1011cm, in line with the expectations for a TypecIIbSN. Together, these diagnostics are difficult to reconcile with the extended radius of the putative yellow supergiant progenitor star identified in archival Hubble Space Telescope observations, unless the stellar density profile is unusual. Finally, we searched for the high-energy shock breakout pulse using X-ray and gamma-ray observations obtained during the purported explosion date range. Based on the compact radius of the progenitor, we estimate that the shock breakout pulse was detectable with current instruments but likely missed due to their limited temporal/spatial coverage. Future all-sky missions will regularly detect shock breakout emission from compact SN progenitors enabling prompt follow-up observations with sensitive multi-wavelength facilities. © 2012. The American Astronomical Society. All rights reserved.
Authors & Co-Authors
Soderberg, Alicia M.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Margutti, Raffaella A.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Zauderer, Bevin Ashley
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Krauss, Miriam I.
United States, Socorro
National Radio Astronomy Observatory Socorro
Katz, B.
United States, Princeton
Institute for Advanced Study
Chomiuk, Laura B.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
United States, Socorro
National Radio Astronomy Observatory Socorro
Dittmann, Jason
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Nakar, Ehud
Israel, Tel Aviv-yafo
Tel Aviv University
Sakamoto, Takanori
United States, Greenbelt
Nasa Goddard Space Flight Center
United States, Baltimore
University of Maryland, Baltimore County Umbc
Kawai, Nobuyuki
Japan, Tokyo
Tokyo Institute of Technology
Hurley, Kevin C.
United States, Berkeley
Space Sciences Laboratory
Barthelmy, Scott D.
United States, Greenbelt
Nasa Goddard Space Flight Center
Toizumi, T.
Japan, Tokyo
Tokyo Institute of Technology
Morii, M.
Japan, Tokyo
Tokyo Institute of Technology
Chevalier, Roger A.
United States, Charlottesville
University of Virginia
Gurwell, Mark A.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Petitpas, Glen R.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Rupen, Michael P.
United States, Socorro
National Radio Astronomy Observatory Socorro
Alexander, Kate D.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Levesque, Emily M.
United States, Boulder
University of Colorado Boulder
Fransson, Claes
Sweden, Stockholm
Stockholms Universitet
Brunthaler, Andreas
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Bietenholz, Michael F.
Canada, Toronto
York University
South Africa, Krugersdorp
Hartebeesthoek Radio Astronomy Observatory
Chugaǐ, N. N. N.
Russian Federation, Moscow
Institute of Astronomy of the Russian Academy of Sciences
Grindlay, Jonathan E.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Copete, A.
United States, Cambridge
Harvard-smithsonian Center for Astrophysics
Connaughton, Valerie
United States, Huntsville
The University of Alabama in Huntsville
Briggs, Michael S.
United States, Huntsville
The University of Alabama in Huntsville
Meegan, Charles A.
United States, Huntsville
Huntsville Program Office
von Kienlin, Andreas
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Zhang, Xiaoling
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Rau, Arne
Germany, Garching Bei Munchen
Max Planck Institute for Extraterrestrial Physics
Golenetskii, S.
Russian Federation, Saint Petersburg
Ioffe Institute
Mazets, E.
Russian Federation, Saint Petersburg
Ioffe Institute
Cline, T.
United States, Greenbelt
Nasa Goddard Space Flight Center
Statistics
Citations: 82
Authors: 35
Affiliations: 18
Identifiers
Doi:
10.1088/0004-637X/752/2/78
ISSN:
0004637X
e-ISSN:
15384357
Research Areas
Environmental
Health System And Policy
Study Design
Cross Sectional Study
Cohort Study