Analysis of information sources in references of the Wikipedia article "GW170817" in Vietnamese language version.
|class= (trợ giúp)The optical and near-infrared spectra over these few days provided convincing arguments that this transient was unlike any other discovered in extensive optical wide-field surveys over the past decade.Đã bỏ qua tham số không rõ
|class= (trợ giúp)Mergers of stellar-mass black holes (BHs) [...] are not expected to have electromagnetic counterparts. [...] I show that the [GW and gamma-ray] signals might be related if the BH binary detected by LIGO originated from two clumps in a dumbbell configuration that formed when the core of a rapidly rotating massive star collapsed.Đã bỏ qua tham số không rõ
|class= (trợ giúp)It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out that the progenitor binary has probably shed a mass ≳10 M☉ during its prior evolution. If even a tiny fraction of this gas is retained in a circumbinary disk, the sudden mass loss and recoil of the merged black hole shocks and heats it within hours of the GW event. Whether the resulting EM signal is detectable is uncertain.Đã bỏ qua tham số không rõ
|class= (trợ giúp)|class= (trợ giúp)|journal= (trợ giúp)|journal= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)|journal= (trợ giúp)|class= (trợ giúp)The optical and near-infrared spectra over these few days provided convincing arguments that this transient was unlike any other discovered in extensive optical wide-field surveys over the past decade.Đã bỏ qua tham số không rõ
|class= (trợ giúp)Mergers of stellar-mass black holes (BHs) [...] are not expected to have electromagnetic counterparts. [...] I show that the [GW and gamma-ray] signals might be related if the BH binary detected by LIGO originated from two clumps in a dumbbell configuration that formed when the core of a rapidly rotating massive star collapsed.Đã bỏ qua tham số không rõ
|class= (trợ giúp)It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out that the progenitor binary has probably shed a mass ≳10 M☉ during its prior evolution. If even a tiny fraction of this gas is retained in a circumbinary disk, the sudden mass loss and recoil of the merged black hole shocks and heats it within hours of the GW event. Whether the resulting EM signal is detectable is uncertain.Đã bỏ qua tham số không rõ
|class= (trợ giúp)|class= (trợ giúp)|journal= (trợ giúp)|journal= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)Mergers of stellar-mass black holes (BHs) [...] are not expected to have electromagnetic counterparts. [...] I show that the [GW and gamma-ray] signals might be related if the BH binary detected by LIGO originated from two clumps in a dumbbell configuration that formed when the core of a rapidly rotating massive star collapsed.Đã bỏ qua tham số không rõ
|class= (trợ giúp)It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out that the progenitor binary has probably shed a mass ≳10 M☉ during its prior evolution. If even a tiny fraction of this gas is retained in a circumbinary disk, the sudden mass loss and recoil of the merged black hole shocks and heats it within hours of the GW event. Whether the resulting EM signal is detectable is uncertain.Đã bỏ qua tham số không rõ
|class= (trợ giúp)The follow-up observers sprang into action, not expecting to detect a signal if the gravitational radiation was indeed from a binary black-hole merger. [...] most observers and theorists agreed: the presence of at least one neutron star in the binary system was a prerequisite for the production of a circumbinary disk or neutron star ejecta, without which no electromagnetic counterpart was expected.
Mergers of stellar-mass black holes (BHs) [...] are not expected to have electromagnetic counterparts. [...] I show that the [GW and gamma-ray] signals might be related if the BH binary detected by LIGO originated from two clumps in a dumbbell configuration that formed when the core of a rapidly rotating massive star collapsed.Đã bỏ qua tham số không rõ
|class= (trợ giúp)It is rare for the birth of a new field of astrophysics to be pinpointed to a singular event. This focus issue follows such an event—the neutron star binary merger GW170817—marking the first joint detection and study of gravitational waves (GWs) and electromagnetic radiation (EM).
It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out that the progenitor binary has probably shed a mass ≳10 M☉ during its prior evolution. If even a tiny fraction of this gas is retained in a circumbinary disk, the sudden mass loss and recoil of the merged black hole shocks and heats it within hours of the GW event. Whether the resulting EM signal is detectable is uncertain.Đã bỏ qua tham số không rõ
|class= (trợ giúp)|class= (trợ giúp)The optical and near-infrared spectra over these few days provided convincing arguments that this transient was unlike any other discovered in extensive optical wide-field surveys over the past decade.Đã bỏ qua tham số không rõ
|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)because colliding black holes don’t give off any light, you wouldn’t expect any optical counterpart.
It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out that the progenitor binary has probably shed a mass ≳10 M☉ during its prior evolution. If even a tiny fraction of this gas is retained in a circumbinary disk, the sudden mass loss and recoil of the merged black hole shocks and heats it within hours of the GW event. Whether the resulting EM signal is detectable is uncertain.Đã bỏ qua tham số không rõ
|class= (trợ giúp)|class= (trợ giúp)|class= (trợ giúp)