Detectibility of mixed unburnt C + O in type Ia supernova spectra - INSPIRE

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Detectibility of mixed unburnt C + O in type Ia supernova spectra

Edward A. Baron
(
- Oklahoma U.
)
,
Eric Lentz
(
- Georgia U.
)
,
Peter H. Hauschildt
(
- Hamburg Observ.
)

Mar, 2003

12 pages

Published in:

Astrophys.J.Lett. 588 (2003) L29-L32

e-Print:

astro-ph/0303627 [astro-ph]

DOI:

10.1086/375526

View in:

ADS Abstract Service

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Abstract: (arXiv)

Motivated by recent 3-D calculations of the explosion of Type Ia supernova via a pure deflagration we calculate the observed spectra at 15-25 days past maximum light of a parameterized model which has a considerable fraction of unburnt C+O in the central regions. Rather than attempting a self consistent 3-D calculation, which is beyond the scope of current computer codes, we modify the composition structure of the 1-D deflagration model W7. In our exploratory parameterized calculations, we find that a central concentration of C+O is not ruled out by observations for the epochs we study. We briefly examine whether nebular phase spectra could be incompatible with observations.

References(28)

Figures(0)

- Mon.Not.Roy.Astron.Soc. 283 297

Infrared and optical spectroscopy of type ia supernovae in the nebular phase

et al.

- Mon.Not.Roy.Astron.Soc. 290 (1997) 663
•
e-Print:
- astro-ph/9707119
•
DOI:
- 10.1093/mnras/290.4.663

- Ann.Rev.Astron.Astrophys. 36 37

On the spectrum and nature of the peculiar type ia supernova 1991t

- Mon.Not.Roy.Astron.Soc. 304 (1999) 67
•
e-Print:
- astro-ph/9807032
•
DOI:
- 10.1046/j.1365-8711.1999.02299.x

- Astrophys.J. 481 L89

Thermonuclear supernovae: Simulations of the deflagration stage and their implications

- Science 299 (2003) 77
•
e-Print:
- astro-ph/0212054
•
DOI:
- 10.1126/science.299.5603.77

Timescale stretch parameterization of Type Ia supernova B-band light curves

Supernova Cosmology Project

Collaboration

•

G. Goldhaber

et al.

- Astrophys.J. 558 (2001) 359-368
•
e-Print:
- astro-ph/0104382
•
DOI:
- 10.1086/322460

The Absolute luminosities of the Calan/Tololo type IA supernovae

et al.

- Astron.J. 112 (1996) 2391
•
e-Print:
- astro-ph/9609059
•
DOI:
- 10.1086/118190

Type Ia supernova explosion models

- Ann.Rev.Astron.Astrophys. 38 (2000) 191-230
•
e-Print:
- astro-ph/0006305
•
DOI:
- 10.1146/annurev.astro.38.1.191

Analysis of the photospheric epoch spectra of Type Ia supernovae SN 1990N and SN 1991T

et al.

- Astrophys.J. 397 (1992) 304-328
•
DOI:
- 10.1086/171787

- Astrophys.J. 419 L77

Three-dimensional modeling of the deflagration stage of a type ia supernova explosion

A.M. Khokhlov

e-Print:
- astro-ph/0008463

- Astrophys.J. 415 589

Nlte synthetic spectral fits to the type ia supernova 1994d in ngc 4526

- Astrophys.J. 557 (2001) 266
•
e-Print:
- astro-ph/0104225
•
DOI:
- 10.1086/322239

On the presence of silicon and carbon in the pre-maximum spectrum of the type ia sn 1990n

Paolo A. Mazzali

- Mon.Not.Roy.Astron.Soc. 321 (2001) 341
•
e-Print:
- astro-ph/0009245
•
DOI:
- 10.1046/j.1365-8711.2001.04018.x

- Astrophys.J. 89 156

Accreting white dwarf models of Type I supernovae. 3. Carbon deflagration supernovae

K. Nomoto
(
- Tokyo U. and
- Garching, Max Planck Inst.
)
,
F.K. Thielemann
(
- Garching, Max Planck Inst.
)
,
K. Yokoi
(
- Karlsruhe U., EKP
)

- Astrophys.J. 286 (1984) 644
•
DOI:
- 10.1086/162639

- Mon.Not.Roy.Astron.Soc. 278 111

Measurements of $\Omega$ and $\Lambda$ from 42 High Redshift Supernovae

Supernova Cosmology Project

Collaboration

•

S. Perlmutter
(
- UC, Berkeley, CfPA
)

et al.

- Astrophys.J. 517 (1999) 565-586
•
e-Print:
- astro-ph/9812133
•
DOI:
- 10.1086/307221

The absolute magnitudes of Type IA supernovae

M.M. Phillips

- Astrophys.J.Lett. 413 (1993) L105-L108
•
DOI:
- 10.1086/186970

The reddening-free decline rate versus luminosity relationship for type ia supernovae

et al.

- Astron.J. 118 (1999) 1766
•
e-Print:
- astro-ph/9907052
•
DOI:
- 10.1086/301032

Thermonuclear explosions of Chandrasekhar-mass C+O white dwarfs

- Astron.Astrophys. 347 (1999) 739
•
e-Print:
- astro-ph/9812120

Observational evidence from supernovae for an accelerating universe and a cosmological constant

et al.

- Astron.J. 116 (1998) 1009-1038
•
e-Print:
- astro-ph/9805201
•
DOI:
- 10.1086/300499

Using SN-Ia light curve shapes to measure the Hubble constant

- Astrophys.J.Lett. 438 (1995) L17-20
•
e-Print:
- astro-ph/9410054
•
DOI:
- 10.1086/187704

A Precise distance indicator: Type Ia supernova multicolor light curve shapes

- Astrophys.J. 473 (1996) 88
•
e-Print:
- astro-ph/9604143
•
DOI:
- 10.1086/178129

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