The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta

Autor: Raffaella Margutti, N. Moskowitz, Matt Nicholl, James Annis, Federica Ricci, Edo Berger, Arash Bahramian, Cesar Briceno, W. Fong, Jay Strader, J. Elias, Ryan Chornock, Ingrid Pelisoli, Tarraneh Eftekhari, Marcelle Soares-Santos, Philip S. Cowperthwaite, Erik Dennihy, D. Brout, Armin Rest, V. A. Villar, B. H. Dunlap, Francesco Massaro, Masao Sako, P. K. Blanchard, Warren R. Brown, Peter K. G. Williams, Kate D. Alexander, Daniel E. Holz, J. C. Clemens, E. J. Marchesini, Brian D. Metzger, Daniel Kasen, Hsin-Yu Chen, Duncan A. Brown
Přispěvatelé: Nicholl, M., Berger, E., Kasen, D., Metzger, B. D., Elias, J., Briceã±o, C., Alexander, K. D., Blanchard, P. K., Chornock, R., Cowperthwaite, P. S., Eftekhari, T., Fong, W., Margutti, R., Villar, V. A., Williams, P. K. G., Brown, W., Annis, J., Bahramian, A., Brout, D., Brown, D. A., Chen, H. -. Y., Clemens, J. C., Dennihy, E., Dunlap, B., Holz, D. E., Marchesini, E., Massaro, F., Moskowitz, N., Pelisoli, I., Rest, A., Ricci, F., Sako, M., Soares-Santos, M., Strader, J., Briceño, C., Chen, H. -.Y.
Jazyk: angličtina
Rok vydání: 2017
Předmět:
close [binaries]
Ciencias Físicas
Astrophysics
Kilonova
7. Clean energy
01 natural sciences
nuclear reaction
Spectral line
purl.org/becyt/ford/1 [https]
nuclear reactions
nucleosynthesis
abundances

Astrophysics::Solar and Stellar Astrophysics
Emission spectrum
Ejecta
010303 astronomy & astrophysics
gravitational wave
Physics
High Energy Astrophysical Phenomena (astro-ph.HE)
abundance
binaries: close
gravitational waves
stars: neutron
Astronomy and Astrophysics
Space and Planetary Science
nucleosynthesis
nuclear reactions
nucleosynthesis
abundance

Astrophysics - Solar and Stellar Astrophysics
nucleosynthesi
Astrophysics::Earth and Planetary Astrophysics
Astrophysics - High Energy Astrophysical Phenomena
CIENCIAS NATURALES Y EXACTAS
Astrophysics - Cosmology and Nongalactic Astrophysics
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
neutron [stars]
Nucleosynthesis
0103 physical sciences
nuclear reactions
Solar and Stellar Astrophysics (astro-ph.SR)
Astrophysics::Galaxy Astrophysics
010308 nuclear & particles physics
Gravitational wave
abundances
Física
purl.org/becyt/ford/1.3 [https]
Astronomy and Astrophysic
Black hole
Astronomía
Neutron star
13. Climate action
Zdroj: SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Popis: We present optical and ultraviolet spectra of the first electromagnetic counterpart to a gravitational-wave (GW) source, the binary neutron star merger GW170817. Spectra were obtained nightly between 1.5 and 9.5 days post-merger, using the Southern Astrophysical Research and Magellan telescopes; the UV spectrum was obtained with the Hubble Space Telescope at 5.5 days. Our data reveal a rapidly fading blue component (T ≈ 5500 K at 1.5 days) that quickly reddens; spectra later than ≳4.5 days peak beyond the optical regime. The spectra are mostly featureless, although we identify a possible weak emission line at ∼7900 Å; at t ≲ 4.5 days. The colors, rapid evolution, and featureless spectrum are consistent with a "blue" kilonova from polar ejecta comprised mainly of light r-process nuclei with atomic mass number A ≲ 140. This indicates a sightline within θobs ≲ 45° of the orbital axis. Comparison to models suggests ∼0.03 M o of blue ejecta, with a velocity of . The required lanthanide fraction is ∼10-4, but this drops to
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Instituto de Astrofísica de La Plata
Databáze: OpenAIRE