215 citations · 1.7k across the 25 of their papers we have counts for
25 papers
The HH 24 Complex: Jets, Multiple Star Formation, and Orphaned Protostars
Bo Reipurth, J. Bally, Hsi-Wei Yen +9
The HH 24 complex harbors five collimated jets emanating from a small protostellar multiple system. We have carried out a multi-wavelength study of the jets, their driving sources,…
High accuracy measurement of gravitational wave back-reaction in the OJ287 black hole binary
Mauri J. Valtonen, L. Dey, R. Hudec +16
Blazar OJ287 exhibits large thermal flares at least twice every 12 years. The times of these flares have been predicted successfully using the model of a quasi-Keplerian eccentric…
Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters
Lankeswar Dey, M. J. Valtonen, A. Gopakumar +5
Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show…
Quasi-satellite dynamics in formation flight
Seppo Mikkola, Claudiu-Lucian Prioroc
The quasi-satellite (QS) phenomenon makes two celestial bodies to fly near each other (Mikkola et al. 2006) and that effect can be used also to make artificial satellites move in t…
Brown Dwarf Binaries from Disintegrating Triple Systems
Bo Reipurth, Seppo Mikkola
We have carried out 200,000 N-body simulations of three identical stellar embryos with masses from a Chabrier IMF and embedded in a molecular core. The bodies are initially non-hie…
Black hole triple dynamics: breakdown of the orbit average approximation and implications for gravitational wave detections
Fabio Antonini, Norman Murray, Seppo Mikkola
Coalescing black hole (BH) binaries forming in the dense core of globular clusters (GCs) are expected to be one the brightest sources of gravitational wave (GW) radiation for the n…