CONTRIBUTIONS OF SHORT-LIVED NUCLIDES BY WOLF-RAYET STARS AND SUPERNOVAE 1b/c TO THE EARLY SOLAR

نویسندگان

  • S. Sahijpal
  • P. Soni
چکیده

1095. [7] Sahijpal (2002) MAPS 65, Abstract #5071. [8] Nomoto et al. (2001) Supernova & Gamma ray bursts. Space Tele. Sci. Symp. Ser. 13, Cambridge Univ. Press 144. [9] Heger et al. astro-ph/0211062. [10] Cerviño et al. (2000) A&A 363, 970. [11] Woosley et al. (1995) Ap.J. 448, 315. [12] Nakamura et al. (2001) Ap.J. 555, 880. [13] Meynet et al. (2001) Space Sci. Rev. 99, 73. [14] Knödlseder et al. (2002) A&A 390, 945. [15] Meynet et al. (1997) A&A 320, 460. [16] Nakamura et al. (2001) Ap.J. 550, 991. [17] Wasserburg et al. (1998) Ap.J. 500, L189. [18] Rauscher et al. (2002) Ap.J. 576, 323. [19] MacPherson et al. (1995) Meteoritics 30, 365. Lunar and Planetary Science XXXIV (2003) 1087.pdf

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Searching for Extinct Chlorine-36 in Enstatite Chondrites: New Constraints on the Distribution of Short-lived Nuclides in the Solar Nebula

Introduction: The origin of short-lived nuclides in the solar nebula is a long standing controversial issue. There are two major explanations: injection from neighboring supernovae or AGB stars [1-3], or in situ irradiation of nebular dust and gas by solar energetic particles (SEP) [4-7]. The distribution of short-lived nuclides in the solar nebula is a key test of these models. Unlike

متن کامل

Constraints on gamma-ray burst and supernova progenitors through circumstellar absorption lines. (II): Post-LBV Wolf-Rayet stars

Context. Wolf-Rayet stars are thought to be the progenitors of Type Ib/c supernovae and of long gamma-ray bursts. Aims. As shown by van Marle et al. (2005), circumstellar absorption lines in early Type Ib/c supernova and gamma-ray burst afterglow spectra may reveal the progenitor evolution of the exploding Wolf-Rayet star. While the quoted paper deals with Wolf-Rayet stars which evolved through...

متن کامل

Star Formation in the Orion-monoceros Complex

Pre-main sequence stars in the Orion-Monoceros Complex are either distributed in groups closed associated with dense cores, or dispersed along molecular filaments. Some molecular clouds are apparently affected by the OrionEridanus Superbubble created by the Wolf-Rayet winds and supernovae from the OriOB1 association, whose shock fronts compressed and triggered starbirth in adjacent molecular cl...

متن کامل

Bayes’ Theorem and Early Solar Short-lived Radionuclides: the Case for an Unexceptional Origin for the Solar System

The presence of excesses of short-lived radionuclides in the early solar system evidenced in meteorites has been taken as testament to close encounters with exotic nucleosynthetic sources, including supernovae or AGB stars. An analysis of the likelihoods associated with different sources of these extinct nuclides in the early solar system indicates that, rather than being exotic, their abundanc...

متن کامل

Short-Lived Nuclei in the Early Solar System: A Low Mass Stellar Source?

We discuss possible stellar origins of short-lived radioactive nuclei with meanlife τ̄≤ 100Myr, which were shown to be alive in the Early Solar System (ESS). We first review current ideas on the production of nuclides having 10≤ τ̄≤ 100Myr, which presumably derive from the continuous interplay of galactic astration, nucleosynthesis from massive supernovae and free decay in the interstellar medium...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003