Type Ia supernovae with and without blueshifted narrow Na I D lines - how different is their structure?

Abstract:
No abstract specified

SEEK ID: https://publications.h-its.org/publications/298

DOI: 10.1093/mnras/stx1578

Research Groups: Physics of Stellar Objects

Publication type: Journal

Journal: Monthly Notices of the Royal Astronomical Society

Citation: Monthly Notices of the Royal Astronomical Society 471(1):491-506

Date Published: 1st Oct 2017

Registered Mode: imported from a bibtex file

Authors: S. Hachinger, F. K. Röpke, P. A. Mazzali, A. Gal-Yam, K. Maguire, M. Sullivan, S. Taubenberger, C. Ashall, H. Campbell, N. Elias-Rosa, U. Feindt, L. Greggio, C. Inserra, M. Miluzio, S. J. Smartt, D. Young

Citation
Hachinger, S., Röpke, F. K., Mazzali, P. A., Gal-Yam, A., Maguire, K., Sullivan, M., Taubenberger, S., Ashall, C., Campbell, H., Elias-Rosa, N., Feindt, U., Greggio, L., Inserra, C., Miluzio, M., Smartt, S. J., & Young, D. (2017). Type Ia supernovae with and without blueshifted narrow Na i D lines – how different is their structure? In Monthly Notices of the Royal Astronomical Society (Vol. 471, Issue 1, pp. 491–506). Oxford University Press (OUP). https://doi.org/10.1093/mnras/stx1578
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Created: 7th Sep 2019 at 11:51

Last updated: 5th Mar 2024 at 21:23

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