Published January 17, 2020 | Version v2

Graphics: Evolutionary pathways leading to Double Neutron Star formation

  • 1. DARK, Niels Bohr Institute

Description

Schematical representations of the evolutionary pathways leading to Double Neutron Stars formation as presented in the paper "Common–Envelope Episodes that lead to Double Neutron Star formation" (arXiv:2001.09829).

Contents:

./Channel_I/
 - 00_Channel_I_circular.pdf   
 - 00_Channel_I_circular.png  
 - 00_Channel_I_vertical.jpg
 - 00_Channel_I_vertical.pdf
 - 00_Channel_I_horizontal.pdf    
 - 00_Channel_I_horizontal.jpg  
 - Channel_I_individual_pdfs.tar.gz
 - Channel_I_individual_pngs.tar.gz

./Channel_II/
 - 00_Channel_II_circular.jpg   
 - 00_Channel_II_circular.pdf    
 - 00_Channel_II_vertical.jpg
 - 00_Channel_II_vertical.pdf
 - 00_Channel_II_horizontal.jpg    
 - 00_Channel_II_horizontal.pdf    
 - Channel_II_individual_pdfs.tar.gz
 - Channel_II_individual_pngs.tar.gz

00_Channel_*_circular.*, 00_Channel_*_vertical.* and 00_Channel_*_horizontal.* contain the figure of the specified formation channel in the specified format in a circular/vertical/horizontal direction.

Channel_*_individual_*.tar.gz contain the individual figures for each formation channel in the specified format.

If you use these illustrations please kindly include a citation to:
A. Vigna-Gómez, M. MacLeod, C. J. Neijssel, F. S. Broekgaarden, S. Justham, G. Howitt, S. E. de Mink, S. Vinciguerra, and I. Mandel. Common envelope episodes that lead to doubleneutron star formation. PASA, 37:e038, Jan. 2020 (ADS)

Files

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