Year |
Citation |
Score |
2018 |
Staff JE, Wiggins B, Marcello D, Motl PM, Even W, Fryer CL, Raskin C, Clayton GC, Frank J. The Role of Dredge-up in Double White Dwarf Mergers The Astrophysical Journal. 862: 74. DOI: 10.3847/1538-4357/Aaca3D |
0.552 |
|
2018 |
Kadam K, Motl PM, Marcello DC, Frank J, Clayton GC. Numerical simulations of mass transfer in binaries with bipolytropic components Monthly Notices of the Royal Astronomical Society. 481: 3683-3707. DOI: 10.1093/Mnras/Sty2540 |
0.599 |
|
2017 |
Motl PM, Frank J, Staff J, Clayton GC, Fryer CL, Even W, Diehl S, Tohline JE. A Comparison of Grid-based and SPH Binary Mass-transfer and Merger Simulations The Astrophysical Journal Supplement Series. 229: 27. DOI: 10.3847/1538-4365/Aa5Bde |
0.584 |
|
2016 |
Lehner L, Liebling SL, Palenzuela C, Motl PM. m=1instability and gravitational wave signal in binary neutron star mergers Physical Review D. 94. DOI: 10.1103/Physrevd.94.043003 |
0.373 |
|
2016 |
Kadam K, Motl PM, Frank J, Clayton GC, Marcello DC. A numerical method for generating rapidly rotating bipolytropic structures in equilibrium Monthly Notices of the Royal Astronomical Society. 462: 2237-2245. DOI: 10.1093/Mnras/Stw1814 |
0.549 |
|
2013 |
Palenzuela C, Lehner L, Ponce M, Liebling SL, Anderson M, Neilsen D, Motl P. Electromagnetic and gravitational outputs from binary-neutron-star coalescence. Physical Review Letters. 111: 061105. PMID 23971553 DOI: 10.1103/Physrevlett.111.061105 |
0.434 |
|
2013 |
Palenzuela C, Lehner L, Liebling SL, Ponce M, Anderson M, Neilsen D, Motl P. Linking electromagnetic and gravitational radiation in coalescing binary neutron stars Physical Review D. 88. DOI: 10.1103/Physrevd.88.043011 |
0.453 |
|
2012 |
Staff JE, Menon A, Herwig F, Even W, Fryer CL, Motl PM, Geballe T, Pignatari M, Clayton GC, Tohline JE. Do r coronae borealis stars form from double white dwarf mergers? Astrophysical Journal. 757. DOI: 10.1088/0004-637X/757/1/76 |
0.39 |
|
2011 |
Neilsen D, Lehner L, Palenzuela C, Hirschmann EW, Liebling SL, Motl PM, Garrett T. Boosting jet power in black hole spacetimes. Proceedings of the National Academy of Sciences of the United States of America. 108: 12641-6. PMID 21768341 DOI: 10.1073/Pnas.1019618108 |
0.355 |
|
2010 |
Chawla S, Anderson M, Besselman M, Lehner L, Liebling SL, Motl PM, Neilsen D. Mergers of magnetized neutron stars with spinning black holes: disruption, accretion, and fallback. Physical Review Letters. 105: 111101. PMID 20867561 DOI: 10.1103/Physrevlett.105.111101 |
0.47 |
|
2009 |
Megevand M, Anderson M, Frank J, Hirschmann EW, Lehner L, Liebling SL, Motl PM, Neilsen D. Perturbed disks get shocked: Binary black hole merger effects on accretion disks Physical Review D - Particles, Fields, Gravitation and Cosmology. 80. DOI: 10.1103/Physrevd.80.024012 |
0.564 |
|
2008 |
Anderson M, Hirschmann EW, Lehner L, Liebling SL, Motl PM, Neilsen D, Palenzuela C, Tohline JE. Magnetized neutron-star mergers and gravitational-wave signals. Physical Review Letters. 100: 191101. PMID 18518432 DOI: 10.1103/Physrevlett.100.191101 |
0.336 |
|
2008 |
Anderson M, Hirschmann EW, Lehner L, Liebling SL, Motl PM, Neilsen D, Palenzuela C, Tohline JE. Simulating binary neutron stars: Dynamics and gravitational waves Physical Review D - Particles, Fields, Gravitation and Cosmology. 77. DOI: 10.1103/Physrevd.77.024006 |
0.478 |
|
2008 |
Jeltema TE, Hallman EJ, Burns JO, Motl PM. Cluster structure in cosmological simulations. I. Correlation to observables, mass estimates, and evolution Astrophysical Journal. 681: 167-186. DOI: 10.1086/587502 |
0.447 |
|
2008 |
Burns JO, Hallman EJ, Gantner B, Motl PM, Norman ML. Why do only some galaxy clusters have cool cores? Astrophysical Journal. 675: 1125-1140. DOI: 10.1086/526514 |
0.407 |
|
2007 |
Motl PM, Frank J, Tohline JE, D'Souza MCR. The stability of double white dwarf binaries undergoing direct-impact accretion Astrophysical Journal. 670: 1314-1325. DOI: 10.1086/522076 |
0.608 |
|
2007 |
Ou S, Tohline JE, Motl PM. Further evidence for an elliptical instability in rotating fluid bars and ellipsoidal stars Astrophysical Journal. 665: 1074-1083. DOI: 10.1086/519785 |
0.41 |
|
2007 |
Hallman EJ, Burns JO, Motl PM, Norman ML. The β-Model problem: The incompatibility of X-ray and sunyaev-zeldovich effect model fitting for galaxy clusters Astrophysical Journal. 665: 911-920. DOI: 10.1086/519447 |
0.316 |
|
2006 |
Rahman N, Krywult J, Motl PM, Flin P, Shandarin SF. Morphology and evolution of simulated and optical clusters: A comparative analysis Monthly Notices of the Royal Astronomical Society. 367: 838-850. DOI: 10.1111/J.1365-2966.2005.10014.X |
0.403 |
|
2006 |
Hallman EJ, Motl PM, Burns JO, Norman ML. Challenges for precision cosmology with X-ray and Sunyaev-Zeldovich effect gas mass measurements of galaxy clusters Astrophysical Journal. 648: 852-867. DOI: 10.1086/505317 |
0.418 |
|
2006 |
D'Souza MCR, Motl PM, Tohline JE, Frank J. Numerical simulations of the onset and stability of dynamical mass transfer in binaries Astrophysical Journal. 643: 381-401. DOI: 10.1086/500384 |
0.605 |
|
2006 |
Motl PM, Tohline JE, Frank J. Angular momentum transport in double white dwarf binaries Aip Conference Proceedings. 873: 422-428. DOI: 10.1063/1.2405079 |
0.465 |
|
2005 |
Motl PM, Hallman EJ, Burns JO, Norman ML. The integrated Sunyaev-zeldovich effect as a superior method for measuring the mass of clusters of galaxies Astrophysical Journal. 623: L63-L66. DOI: 10.1086/430144 |
0.411 |
|
2004 |
Floor SN, Melott AL, Motl PM. Simulated versus observed cluster eccentricity evolution Astrophysical Journal. 611: 153-157. DOI: 10.1086/422090 |
0.411 |
|
2004 |
Motl PM, Burns JO, Loken C, Norman ML, Bryan G. Formation of cool cores in galaxy clusters via hierarchical mergers Astrophysical Journal. 606: 635-653. DOI: 10.1086/381566 |
0.438 |
|
2002 |
Loken C, Norman ML, Nelson E, Burns J, Bryan GL, Motl P. A universal temperature profile for galaxy clusters Astrophysical Journal. 579: 571-576. DOI: 10.1086/342825 |
0.417 |
|
2002 |
Motl PM, Tohline JE, Frank J. Numerical methods for the simulation of dynamical mass transfer in binaries Astrophysical Journal, Supplement Series. 138: 121-148. DOI: 10.1086/324159 |
0.596 |
|
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