SN 2008am: A Super-Luminous Type IIn Supernova

dc.contributor.utaustinauthorChatzopoulos, E.en_US
dc.contributor.utaustinauthorWheeler, J. Craigen_US
dc.contributor.utaustinauthorRobinson, Edward L.en_US
dc.creatorChatzopoulos, Emmanouilen_US
dc.creatorWheeler, J. Craigen_US
dc.creatorVinko, Jozsefen_US
dc.creatorQuimby, Roberten_US
dc.creatorRobinson, Edward L.en_US
dc.creatorMiller, A. A.en_US
dc.creatorFoley, Ryan J.en_US
dc.creatorPerley, D. A.en_US
dc.creatorYuan, F.en_US
dc.creatorAkerlof, C.en_US
dc.creatorBloom, Joshua S.en_US
dc.date.accessioned2016-04-28T19:31:55Z
dc.date.available2016-04-28T19:31:55Z
dc.date.issued2011-03en
dc.description.abstractWe present observations and interpretation of the Type IIn supernova SN 2008am discovered by the ROTSE Supernova Verification Project (RSVP). SN 2008am peaked at approximately -22.3 mag at a redshift of z = 0.2338, giving it a peak luminosity of similar to 3 x 10(44) erg s(-1) and making it one of the most luminous supernovae ever observed. The total radiated energy is similar or equal to 2 x 10(51) erg. The host galaxy appears to be an SB1 of normal luminosity (M-r' similar to -20) with metallicity Z similar to 0.4Z(circle dot). ROTSE upper limits and detections constrain the rise time to be similar to 34 days in the rest frame, significantly shorter than similar events, SN 2006gy and SN 2006tf. Photometric observations in the ultraviolet, optical, and infrared bands (J, H, K-s) constrain the spectral energy distribution evolution. We obtained six optical spectra of the supernova, five on the early decline from maximum light and a sixth nearly a year later plus a very late time spectrum (similar to 2 yr) of the host galaxy. The spectra show no evidence for broad supernova photospheric features in either absorption or emission at any phase. The spectra of SN 2008am show strong Balmer-line and He I lambda 5876 emission with intermediate widths (similar to 25 angstrom) in the first similar to 40 days after optical maximum. The width formally corresponds to a velocity of similar to 1000 km s(-1). We examine a variety of models for the line wings and conclude that multiple scattering is most likely, implying that our spectra contain no specific information on the bulk flow velocity. We examine a variety of models for the ROTSE light curve subject to the rise time and the nature of the spectra, including radioactive decay, shocks in optically thick and optically thin circumstellar media (CSMs) and a magnetar. The most successful model is one for which the CSM is optically thick and in which diffusion of forward shock-deposited luminosity gives rise to the observed light curve. The model suggests strong mass loss and a greater contribution from the interaction of the forward shock with optically thick CSM than from the reverse shock. Diffusion of the shock-deposited energy from the forward shock is found to be important in accounting for the rising part of the light curve. Although there are differences in detail, SN 2008am appears to be closely related to other super-luminous Type IIn supernovae, SN 2006gy, SN 2006tf, and perhaps SN 2008iy, that may represent the deaths of very massive luminous-blue-variable-type progenitors and for which the luminosity is powered by the interaction of the ejecta with a dense CSM.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipNSF AST-0707669en_US
dc.description.sponsorshipTexas Advanced Research Program ASTRO-ARP-0094en_US
dc.description.sponsorshipPropondis foundation of Piraeus, Greeceen_US
dc.description.sponsorshipHungarian OTKA K76816en_US
dc.identifierdoi:10.15781/T21F8W
dc.identifier.Filename2011_03_sn2008am.pdfen_US
dc.identifier.citationChatzopoulos, E., J. Craig Wheeler, J. Vinko, R. Quimby, E. L. Robinson, A. A. Miller, R. J. Foley et al. "SN 2008am: a super-luminous Type IIn supernova." The Astrophysical Journal, Vol. 729, No. 2 (Mar., 2011): 143.en_US
dc.identifier.doi10.1088/0004-637x/729/2/143en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/2152/34656
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journalen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectcircumstellar matteren_US
dc.subjecthydrodynamicsen_US
dc.subjectstars: evolutionen_US
dc.subjectsupernovae:en_US
dc.subjectgeneralen_US
dc.subjectsupernovae: individual (sn 2008am)en_US
dc.subjectrich circumstellar mediumen_US
dc.subjectcore-collapse supernovaeen_US
dc.subjectpair-instabilityen_US
dc.subjectlight-curveen_US
dc.subjectmassive starsen_US
dc.subjectelectron-scatteringen_US
dc.subjectphotometric systemen_US
dc.subjectanalytic solutionsen_US
dc.subjecttelescope systemen_US
dc.subjectspace-telescopeen_US
dc.subjectastronomy & astrophysicsen_US
dc.titleSN 2008am: A Super-Luminous Type IIn Supernovaen_US
dc.typeArticleen_US

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