Central Cluster Galaxies: A Hot Spot for Detectable Gravitational Waves from Black Hole Mergers
Since pulsar timing arrays (PTAs) announced the evidence for a low-frequency gravitational-wave (GW) background, continuous waves (CWs) have been the next anticipated GW signals. In this work, we model CW sources detectable by PTAs based on the massive black hole (MBH) merger population in the ASTRI...
Gorde:
| Egile Nagusiak: | , , , , , , , , |
|---|---|
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
IOP Publishing
2025-01-01
|
| Saila: | The Astrophysical Journal Letters |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/2041-8213/adf101 |
| Etiketak: |
Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!
|