activity
19962023
most citedPSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

1.8k citations · 4.3k across the 34 of their papers we have counts for

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Showing 2003 · astro-phShow all

5 papers · 2 filters

astro-ph2003

Interpreting QPOs from Accreting Neutron Stars

M. Coleman Miller

The high time resolution and large area of the Rossi X-ray Timing Explorer have been essential in the detection and characterization of high-frequency quasi-periodic variability in…

astro-ph2003

Revealing a Cool Accretion Disk in the Ultraluminous X-ray Source M81 X-9 (Holmberg IX X-1): Evidence for an Intermediate Mass Black Hole

J. M. Miller, A. C. Fabian, M. C. Miller

We report the results of an analysis of two XMM-Newton/EPIC-pn spectra of the bright ultraluminous X-ray source M81 X-9 (Holmberg IX X-1), obtained in snapshot observations. Soft t…

astro-ph2003★ 14 cited

Sonic-Point and Spin-Resonance Model of the Kilohertz QPO Pairs

Frederick K. Lamb, M. Coleman Miller

KHz QPOs have now been detected in more than twenty accreting neutron stars in low-mass binary systems. Two kHz QPOs are usually detected in each star. Burst oscillations and two k…

astro-ph2003

Three-Body Encounters of Black Holes in Globular Clusters

Kayhan Gultekin, M. Coleman Miller, Douglas P. Hamilton

Evidence has been mounting for the existence of black holes with masses from 10^2 to 10^4 M_Solar associated with stellar clusters. Such intermediate-mass black holes (IMBHs) will…

astro-ph2003

Formation Scenarios for Intermediate-Mass Black Holes

M. Coleman Miller

Black holes with hundreds to thousands of solar masses are more massive than can be formed from a single star in the current universe, yet the best candidates for these objects are…