Author | dc.contributor.author | Cartier Ugarte, Regis | |
Author | dc.contributor.author | Hamuy Wackenhut, Mario | es_CL |
Author | dc.contributor.author | Pignata Libralato, Giuliano | es_CL |
Author | dc.contributor.author | Förster, Francisco | es_CL |
Author | dc.contributor.author | Zelaya, Paula | es_CL |
Author | dc.contributor.author | Folatelli, Gastón | es_CL |
Author | dc.contributor.author | Phillips, Mark M. | es_CL |
Author | dc.contributor.author | Morrell, Nidia | es_CL |
Author | dc.contributor.author | Krisciunas, Kevin | es_CL |
Author | dc.contributor.author | Suntzeff, Nicholas B. | es_CL |
Author | dc.contributor.author | Clocchiatti, Alejandro | es_CL |
Author | dc.contributor.author | Coppi, Paolo | es_CL |
Author | dc.contributor.author | Contreras, Carlos | es_CL |
Author | dc.contributor.author | Roth, Miguel | es_CL |
Author | dc.contributor.author | Koviak, Kathleen | es_CL |
Author | dc.contributor.author | Maza Sancho, José | es_CL |
Author | dc.contributor.author | González, Luis | es_CL |
Author | dc.contributor.author | González, Sergio | |
Author | dc.contributor.author | Huerta, Leonor | |
Admission date | dc.date.accessioned | 2014-09-16T13:26:01Z | |
Available date | dc.date.available | 2014-09-16T13:26:01Z | |
Publication date | dc.date.issued | 2014-07-01 | |
Cita de ítem | dc.identifier.citation | The Astrophysical Journal, 789:89 (22pp), 2014 July 1 | en_US |
Identifier | dc.identifier.other | doi:10.1088/0004-637X/789/1/89 | |
Identifier | dc.identifier.uri | https://repositorio.uchile.cl/handle/2250/126472 | |
General note | dc.description | Artículo de publicación ISI. | en_US |
Abstract | dc.description.abstract | We present well-sampled UBVRIJHK photometry of SN 2002fk starting 12 days before maximum light through
122 days after peak brightness, along with a series of 15 optical spectra from −4 to +95 days since maximum. Our
observations show the presence of C ii lines in the early-time spectra of SN 2002fk, expanding at 11,000 km s−1 and persisting until 8 days past maximum light with a velocity of ∼9000 km s−1. SN 2002fk is characterized
by a small velocity gradient of v˙Si ii = 26 km s−1 day−1, possibly caused by an off-center explosion with the ignition region oriented toward the observer. The connection between the viewing angle of an off-center explosion
and the presence of C ii in the early-time spectrum suggests that the observation of Cii could be also due to a
viewing angle effect. Adopting the Cepheid distance to NGC 1309 we provide the first H0 value based on near infrared (near-IR) measurements of a Type Ia supernova (SN) between 63.0 ± 0.8 (±3.4 systematic) and 66.7 ± 1.0
(±3.5 systematic) km s−1 Mpc−1, depending on the absolute magnitude/decline rate relationship adopted. It appears
that the near-IR yields somewhat lower (6%–9%) H0 values than the optical. It is essential to further examine this issue by (1) expanding the sample of high-quality near-IR light curves of SNe in the Hubble flow, and (2) increasing
the number of nearby SNe with near-IR SN light curves and precise Cepheid distances, which affords the promise to deliver a more precise determination of H0. | en_US |
Lenguage | dc.language.iso | en_US | en_US |
Publisher | dc.publisher | The American Astronomical Society | en_US |
Keywords | dc.subject | Key words: cosmological parameters | en_US |
Título | dc.title | Persistent Cii Absorption In the Normal TYPE Ia Supernova 2002fk∗ | en_US |
Document type | dc.type | Artículo de revista | |