Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Timmes, Frank X."'
Publikováno v:
Proc. IAU 14 (2018) 449-454
The discovery via gravitational waves of binary black hole systems with total masses greater than $60M_\odot$ has raised interesting questions for stellar evolution theory. Among the most promising formation channels for these systems is one involvin
Externí odkaz:
http://arxiv.org/abs/1811.03656
Autor:
Arcones, Almudena, Bardayan, Dan W., Beers, Timothy C., Berstein, Lee A., Blackmon, Jeffrey C., Messer, Bronson, Brown, B. Alex, Brown, Edward F., Brune, Carl R., Champagne, Art E., Chieffi, Alessandro, Couture, Aaron J., Danielewicz, Pawel, Diehl, Roland, El-Eid, Mounib, Escher, Jutta, Fields, Brian D., Fröhlich, Carla, Herwig, Falk, Hix, William Raphael, Iliadis, Christian, Lynch, William G., McLaughlin, Gail C., Meyer, Bradley S., Mezzacappa, Anthony, Nunes, Filomena, O'Shea, Brian W., Prakash, Madappa, Pritychenko, Boris, Reddy, Sanjay, Rehm, Ernst, Rogachev, Grigory, Rutledge, Robert E., Schatz, Hendrik, Smith, Michael S., Stairs, Ingrid H., Steiner, Andrew W., Strohmayer, Tod E., Timmes, Frank X., Townsley, Dean M., Wiescher, Michael, Zegers, Remco G. T., Zingale, Michael
This white paper informs the nuclear astrophysics community and funding agencies about the scientific directions and priorities of the field and provides input from this community for the 2015 Nuclear Science Long Range Plan. It summarizes the outcom
Externí odkaz:
http://arxiv.org/abs/1603.02213
Autor:
Jones, Samuel, Hirschi, Raphael, Nomoto, Ken'ichi, Fischer, Tobias, Timmes, Frank X., Herwig, Falk, Paxton, Bill, Toki, Hiroshi, Suzuki, Toshio, Martinez-Pinedo, Gabriel, Lam, Yi Hua, Bertolli, Michael G.
Publikováno v:
ApJ, 772, 150 (2013)
The stellar mass range 8
Externí odkaz:
http://arxiv.org/abs/1306.2030
Autor:
Bennett, Michael E., Hirschi, Raphael, Pignatari, Marco, Diehl, Steven, Fryer, Chris, Herwig, Falk, Hillary, William, Hungerford, Aimee, Richman, Debra, Rockefeller, Gabriel, Timmes, Frank X., Wiescher, Michael
The contribution by massive stars (M > 9 solar masses) to the weak s-process component of the solar system abundances is primarily due to the 22Ne neutron source, which is activated near the end of helium-core burning. The residual 22Ne left over fro
Externí odkaz:
http://arxiv.org/abs/1012.3258
Autor:
Diehl, Roland, Timmes, Frank X.
Publikováno v:
AIP Conference Proceedings; May1997, Vol. 410 Issue 1, p218-248, 31p
Publikováno v:
AIP Conference Proceedings; 2006, Vol. 847 Issue 1, p467-469, 3p, 2 Diagrams
Autor:
Hinkel, Natalie R.
The only elements that were made in significant quantity during the Big Bang were hydrogen and helium, and to a lesser extent lithium. Depending on the initial mass of a star, it may eject some or all of the unique, newly formed elements into the int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b6b3e234b68d9e7f74c6fd6a526addc