Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26865
Titolo: | The unpolarized macronova associated with the gravitational wave event GW 170817 | Autori: | COVINO, Stefano Wiersema, K. Fan, Y. Z. Toma, K. Higgins, A. B. MELANDRI, Andrea D'AVANZO, Paolo Mundell, C. G. PALAZZI, ELIANA Tanvir, N. R. BERNARDINI, Maria Grazia Branchesi, M. BROCATO, Enzo CAMPANA, Sergio di Serego Alighieri, S. Götz, D. Fynbo, J. P. U. Gao, W. Gomboc, A. Gompertz, B. Greiner, J. Hjorth, J. Jin, Z. P. Kaper, L. Klose, S. Kobayashi, S. Kopac, D. Kouveliotou, C. Levan, A. J. Mao, J. Malesani, D. PIAN, Elena ROSSI, Andrea SALVATERRA, Ruben Starling, R. L. C. Steele, I. TAGLIAFERRI, Gianpiero Troja, E. van der Horst, A. J. Wijers, R. A. M. J. |
Data pubblicazione: | 2017 | Rivista: | NATURE ASTRONOMY | Numero: | 1 | Da pagina:: | 791 | Abstract: | The merger of two dense stellar remnants including at least one neutron star is predicted to produce gravitational waves (GWs) and short-duration gamma ray bursts<SUP>1,2</SUP>. In the process, neutron-rich material is ejected from the system and heavy elements are synthesized by r-process nucleosynthesis<SUP>1,3</SUP>. The radioactive decay of these heavy elements produces additional transient radiation termed kilonova or macronova<SUP>4-10</SUP>. We report the detection of linear optical polarization, P = (0.50 ± 0.07)%, 1.46 days after detection of the GWs from GW 170817—a double neutron star merger associated with an optical macronova counterpart and a short gamma ray burst<SUP>11-14</SUP>. The optical emission from a macronova is expected to be characterized by a blue, rapidly decaying component and a red, more slowly evolving component due to material rich in heavy elements—the lanthanides<SUP>15</SUP>. The polarization measurement was made when the macronova was still in its blue phase, during which there was an important contribution from a lanthanide-free outflow. The low degree of polarization is consistent with intrinsically unpolarized emission scattered by galactic dust, suggesting a symmetric geometry of the emitting region and low inclination of the merger system. Stringent upper limits to the polarization degree from 2.45-9.48 days post-burst are consistent with the lanthanides-rich macronova interpretation. | URI: | http://hdl.handle.net/20.500.12386/26865 | URL: | https://www.nature.com/articles/s41550-017-0285-z | ISSN: | 2397-3366 | DOI: | 10.1038/s41550-017-0285-z | Bibcode ADS: | 2017NatAs...1..791C | Fulltext: | open |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
1710.05849 | preprint | 226.08 kB | Adobe PDF | Visualizza/apri |
s41550-017-0285-z.pdf | [Administrators only] | 1.1 MB | Adobe PDF |
Page view(s)
80
controllato il 24-apr-2024
Download(s)
25
controllato il 24-apr-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.