Abundances of Sodium (Na) and Europium (Eu) in bulge field stars
Milky Way's disk structures as a memory of its turbulent past
| Full text | |
| Author(s): |
Horvath, J. E.
[1]
;
Benvenuto, O. G.
[2, 3]
;
Bauer, E.
[4, 2]
;
Paulucci, L.
[5]
;
Bernardo, A.
[1]
;
Viturro, H. R.
[2]
Total Authors: 6
|
| Affiliation: | [1] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, R Matao 1226, BR-05508090 Sao Paulo, SP - Brazil
[2] Univ Nacl La Plata, Fac CienciasAstron & Geofis, Paseo Bosque S-N, RA-1900 La Plata - Argentina
[3] Univ Nacl La Plata, Inst Astrofis La Plata, Paseo Bosque S-N, RA-1900 La Plata - Argentina
[4] Consejo Nacl Invest Cient & Tecn, Inst Fis La Plata, RA-1900 La Plata - Argentina
[5] Univ Fed Abc, Av Estados 5001, BR-09210170 Santo Andre, SP - Brazil
Total Affiliations: 5
|
| Document type: | Journal article |
| Source: | UNIVERSE; v. 5, n. 6 JUN 2019. |
| Web of Science Citations: | 0 |
| Abstract | |
In this talk, we summarize the work in progress toward a full characterization of strange star-strange star (SS-SS) mergers related to the GW/GRB/kilonova events. In addition, we show that the a priori probability constructed from the observed neutron star mass distribution points toward an asymmetric binary system as the progenitor of the GW170817 event. (AU) | |
| FAPESP's process: | 13/26258-4 - Superdense matter in the universe |
| Grantee: | Manuel Máximo Bastos Malheiro de Oliveira |
| Support Opportunities: | Research Projects - Thematic Grants |