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20032025
most citedGalactic chemical evolution: Carbon through Zinc

890 citations · 10.3k across the 163 of their papers we have counts for

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Showing 2008Show all

11 papers · 1 filter

astro-ph2008★ 1 cited

Origin and Nature of Dust in the Early Universe

T. Nozawa, T. Kozasa, H. Umeda +8

We present recent advances in theoretical studies of the formation and evolution of dust in primordial supernovae (SNe) that are considered to be the main sources of dust in the ea…

astro-ph2008★ 42 cited

Optical photometry and spectroscopy of the type Ibn supernova SN 2006jc until the onset of dust formation

G. C. Anupama, D. K. Sahu, U. K. Gurugubelli +4

We present optical UBVRI photometric and spectroscopic data of the type Ibn supernova SN 2006jc, until the onset of the dust forming phase. The optical spectrum shows a blue contin…

astro-ph2008★ 42 cited

Explosive Nucleosynthesis of Weak r-Process Elements in Extremely Metal-Poor Core-Collapse Supernovae

N. Izutani, H. Umeda, N. Tominaga

There have been attempts to fit the abundance patterns of extremely metal-poor stars with supernova nucleosynthesis models for the lighter elements than Zn. On the other hand, obse…

astro-ph2008

Supernova Nucleosynthesis and Extremely Metal-Poor Stars

Nozomu Tominaga, Hideyuki Umeda, Keiichi Maeda +2

We investigate hydrodynamical and nucleosynthetic properties of the jet-induced explosion of a population III star and compare the abundance patterns of the yields with…

astro-ph2008

Evolution of newly formed dust in Population III supernova remnants and its impact on the elemental composition of Population II.5 stars

Takaya Nozawa, Takashi Kozasa, Asao Habe +5

We investigate the evolution of dust formed in Population III supernovae (SNe) by considering its transport and processing by sputtering within the SN remnants (SNRs). We find that…

astro-ph2008

Supernova Nucleosynthesis in the Early Universe

Nozomu Tominaga, Hideyuki Umeda, Keiichi Maeda +2

The first metal enrichment in the universe was made by supernova (SN) explosions of population (Pop) III stars. The trace remains in abundance patterns of extremely metal-poor (EMP…

astro-ph2008★ 60 cited

Injection of Short-Lived Radionuclides into the Early Solar System from a Faint Supernova with Mixing-Fallback

A. Takigawa, J. Miki, S. Tachibana +4

Several short-lived radionuclides (SLRs) were present in the early solar system, some of which should have formed just prior to or soon after the solar system formation. Stellar nu…

astro-ph2008★ 258 cited

The metamorphosis of Supernova SN2008D/XRF080109: a link between Supernovae and GRBs/Hypernovae

Paolo A. Mazzali, Stefano Valenti, Massimo Della Valle +38

The only supernovae (SNe) to have shown early gamma-ray or X-ray emission thus far are overenergetic, broad-lined Type Ic SNe (Hypernovae - HNe). Recently, SN 2008D shows several n…

astro-ph2008★ 91 cited

Type Ib Supernova 2008D associated with the Luminous X-ray Transient 080109: An Energetic Explosion of a Massive Helium Star

Masaomi Tanaka, Nozomu Tominaga, Ken'ichi Nomoto +11

We present a theoretical model for supernova (SN) 2008D associated with the luminous X-ray transient 080109. The bolometric light curve and optical spectra of the SN are modelled b…

astro-ph2008★ 50 cited

Chemical Abundances of the Secondary Star in the Black Hole X-ray Binary XTE J1118+480

Jonay I. González Hernández, Rafael Rebolo, Garik Israelian +5

Following the recent abundance measurements of Mg, Al, Ca, Fe, and Ni in the black hole X-ray binary XTE J1118+480 using medium-resolution Keck II/ESI spectra of the secondary star…

astro-ph2008★ 83 cited

Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and Temperature and Mass of the Dust

T. Nozawa, T. Kozasa, N. Tominaga +8

SN 2006jc is a peculiar supernova (SN), in which the formation of dust has been confirmed at an early epoch of ~50 days after the explosion. We investigate the possibility of such…