Globular clusters house a population of compact binaries that will be interesting gravitational wave sources for LISA. We provide estimates for the numbers of sources of several categories and discuss the sensitivity of LISA to detecting these sources. The estimated total number of detectable sources ranges from ∼10 to∼103 with gravitational wave frequencies above 1 mHz. These sources are typically undetectable by any other means and thus offer an opportunity for doing true gravitational-wave astronomy. The detection of these sources would provide information about both binary star evolution and the dynamics of globular clusters. PACS numbers: 0430D, 0480N, 9555Y, 9780, 9820G 1
Abstract. With full-sensitivity operation of the first generation of gravitational wave detectors no...
Aims. We present the first fully relativistic study of gravitational radiation from bodies in circul...
The sources of gravitational radiation that seem to be most likely to be detected by planned ground-...
I review the expected Galactic sources of gravitational waves, concentrating on the low-frequency do...
The detection of gravitational-waves emitted by double compact objects is starting to inform our und...
Contains fulltext : 35803.pdf (publisher's version ) (Closed access)I ll give an o...
Abstract. The sources of gravitational radiation that seem to be most likely to be detected by plann...
International audienceWe study the evolution and gravitational wave emission of white dwarf–black ho...
Future searches for gravitational waves from space will be sensitive to double compact objects in ou...
Space-based gravitational wave detectors will have the ability to observe continuous low-frequency g...
The rapid advance of gravitational-wave (GW) detector facilities makes it very important to estimate...
International audienceMultiband observations of coalescing stellar-mass black holes binaries could d...
The rapid advance of gravitational-wave (GW) detector facilities makes it very important to estimate...
The world wide efforts for detecting gravitational waves, the detectors in vogue and the expected as...
Gravitational wave detectors in space, particularly the LISA project, can study a rich variety of as...
Abstract. With full-sensitivity operation of the first generation of gravitational wave detectors no...
Aims. We present the first fully relativistic study of gravitational radiation from bodies in circul...
The sources of gravitational radiation that seem to be most likely to be detected by planned ground-...
I review the expected Galactic sources of gravitational waves, concentrating on the low-frequency do...
The detection of gravitational-waves emitted by double compact objects is starting to inform our und...
Contains fulltext : 35803.pdf (publisher's version ) (Closed access)I ll give an o...
Abstract. The sources of gravitational radiation that seem to be most likely to be detected by plann...
International audienceWe study the evolution and gravitational wave emission of white dwarf–black ho...
Future searches for gravitational waves from space will be sensitive to double compact objects in ou...
Space-based gravitational wave detectors will have the ability to observe continuous low-frequency g...
The rapid advance of gravitational-wave (GW) detector facilities makes it very important to estimate...
International audienceMultiband observations of coalescing stellar-mass black holes binaries could d...
The rapid advance of gravitational-wave (GW) detector facilities makes it very important to estimate...
The world wide efforts for detecting gravitational waves, the detectors in vogue and the expected as...
Gravitational wave detectors in space, particularly the LISA project, can study a rich variety of as...
Abstract. With full-sensitivity operation of the first generation of gravitational wave detectors no...
Aims. We present the first fully relativistic study of gravitational radiation from bodies in circul...
The sources of gravitational radiation that seem to be most likely to be detected by planned ground-...