Search - Virtual Journal of Nuclear Astrophysics

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Results 1 - 9 of 9

Gas-phase Fe/O and Fe/N abundances in Star-Forming Regions. Relations between nucleosynthesis, metallicity and dust
- Virtual Journal - Volume 22, Issue 33 - article #6
- J. E. M'endez-Delgado, K. Kreckel, C. Esteban, J. Garc'ia-Rojas, L. Carigi, A. A. C. Sander, M. Palla, M. Chru'sli'nska, I. De Looze, M. Rela~no, S. A. van der Giessen, E. Reyes-Rodr'iguez, S. F. S'anchez
- https://arxiv.org/abs/2408.06215
Optically-thick Structure in Early B Type Supergiant Stellar Winds at Low Metallicities. (arXiv:2401.01240v1 [astro-ph.SR])
- Virtual Journal - Volume 22, Issue 1 - article #10
- Timothy N. Parsons, Raman K. Prinja, Matheus Bernini-Peron, Alex W. Fullerton, Derck L. Massa, Lidia M. Oskinova, Daniel Pauli, Andreas A.C. Sander, Matthew J. Rickard
- http://arxiv.org/abs/2401.01240
Very Massive Stars and Pair-Instability Supernovae: Mass-loss Framework for low Metallicity. (arXiv:2306.11785v1 [astro-ph.SR])
- Virtual Journal - Volume 21, Issue 25 - article #6
- Gautham N. Sabhahit, Jorick S. Vink, Andreas A.C. Sander, Erin R. Higgins
- http://arxiv.org/abs/2306.11785
A partially stripped massive star in a Be binary at low metallicity: A missing link towards Be X-ray binaries and double neutron star mergers. (arXiv:2305.14262v1 [astro-ph.SR])
- Virtual Journal - Volume 21, Issue 21 - article #1
- V. Ramachandran, J. Klencki, A. A. C. Sander, D. Pauli, T. Shenar, L. M. Oskinova, W.-R. Hamann
- http://arxiv.org/abs/2305.14262
Revisiting the archetypical wind accretor Vela X-1 in depth -- A case study of a well-known X-ray binary and the limits of our knowledge. (arXiv:2104.13148v2 [astro-ph.HE] UPDATED)
- Virtual Journal - Volume 19, Issue 20 - article #10
- Peter Kretschmar, Ileyk El Mellah, Silvia Martínez-Núñez, Felix Fürst, Victoria Grinberg, Andreas A. C. Sander, Jakob van den Eijnden, Nathalie Degenaar, Jesús Maíz-Apellániz, Francisco Jiménez Esteban, Mercedes Ramos-Lerate, Enrique Utrilla
- http://arxiv.org/abs/2104.13148
Why binary interaction does not necessarily dominate the formation of Wolf-Rayet stars at low metallicity
- Virtual Journal - Volume 18, Issue 7 - article #10
- T. Shenar, A. Gilkis, J. S. Vink, H. Sana, A. A. C. Sander
- Astronomy & Astrophysics
- http://feedproxy.google.com/~r/edp_aa/~3/UjaWUbUUCfY/201936948
Vela X-1 as a laboratory for accretion in High-Mass X-ray Binaries. (arXiv:1905.08578v1 [astro-ph.HE])
- Virtual Journal - Volume 17, Issue 21 - article #7
- P. Kretschmar, S. Martínez-Núñez, F. Fürst, V. Grinberg, M. Lomaeva, I. El Mellah, A. Manousakis, A. A. C. Sander, N. Degenaar, J. van den Eijnden
- http://arxiv.org/abs/1905.08578
Testing massive star evolution, star formation history, and feedback at low metallicity
- Virtual Journal - Volume 17, Issue 21 - article #10
- V. Ramachandran, W.-R. Hamann, L. M. Oskinova, J. S. Gallagher, R. Hainich, T. Shenar, A. A. C. Sander, H. Todt, L. Fulmer
- Astronomy & Astrophysics
- http://feedproxy.google.com/~r/edp_aa/~3/LG2o2caE0II/201935365
A new Determination of the Extragalactic Background of Diffuse Gamma Rays taking into account Dark Matter Annihilation
- Virtual Journal - Volume 5, Issue 18 - article #22
- W. de Boer, A. Nordt, C. Sander, V. Zhukov (University of Karlsruhe, Germany)
- ArXiv - Astrophysics
- arXiv:0705.0094 [ps, pdf, other]

Results 1 - 9 of 9

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