Radiative Processes In Astrophysics

By C. Freytag. 2016

2,000 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/ee21979e71c4906e080fd2868031a781df460619

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Bing Zhang
2. T. Birnstiel
3. D. Wilner
4. S. Andrews
5. Xue-Ning Bai
6. C. Dullemond
7. Zhaohuan Zhu
8. Pawan Kumar

In Atomic and Molecular Physics, and Optics

1. Xue-Ning Bai
2. Bing Zhang
3. S. Vagnozzi
4. S. Glover
5. T. Birnstiel
6. F. Camilo
7. R. Essig
8. Jae Hyeok Chang

In Instrumentation

1. S. Andrews
2. T. Birnstiel
3. D. Wilner
4. Xue-Ning Bai
5. Zhaohuan Zhu
6. J. Carpenter
7. C. Dullemond
8. L. P'erez

Citations in the corpus

• First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole (2019, neutral): “The set of four possible cross-correlations among the two recorded polarizations at the two sites then provides information about the four Stokes parameters (see, e.g., Roberts et al. 1994).”
• The nebular spectra of SN 2012aw and constraints on stellar nucleosynthesis from oxygen emission lines (2013, methodology): “First, we replace the nonrelativistic Doppler formula with the relativistic one (e.g. Rybicki & Lightman 1979) λ = λ′γ(V ) ( 1− V c cos θ ) (1) where λ and λ′ are the wavelengths in the two frames, V is the relative velocity, θ is the angle (between the direction of the photon and the velocity), c…”
• COSMOLOGICAL IMPLICATIONS OF FAST RADIO BURST/GAMMA-RAY BURST ASSOCIATIONS (2013, methodology): “(8) Based on the above equations, we calculate the rest frame GRB DM value, DMGRB,z for a set of typical values of GRB parameters (Panaitescu & Kumar 2002; Yost et al. 2003; Zhang & Mészáros 2004): r1 = 10 7 cm, Eiso = 10 53 erg, Γ0 = 300 (so that M0 = 3.7 × 10 29 g), δt = 500 s, n = 1 cm−3 (ISM)…”
• A hadronic origin for ultra-high-frequency-peaked BL Lac objects (2014, methodology): “…but we will refer to it simply as ”electrons” in the following. relativistic formulae for the emissivity and self-absorption (see for example Rybicki & Lightman 1979); the inverse Compton emission is evaluated using the Compton kernel given by Jones (1968), which correctly describes the…”
• The physics of gamma-ray bursts & relativistic jets (2014, background): “There are a number of excellent articles that discussmultiple-IC scatterings and the emergent spectrumat great depth [585,586,123,587,588].”
• GIANT SPARKS AT COSMOLOGICAL DISTANCES? (2014, methodology): “Here, ωB = eB/(γmec) is the gyro-frequency of an electron with Lorenz factor γ and gyrating in a magnetic field of strength B and moving in the mean at an angle α with respect to the field lines (Rybicki & Lightman 1979, Chapter 6).”
• Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra (2017, methodology): “Mass and radius values on this line correspond to the solutions that are close to the maximum distance attainable for the system (see e.g., Appendix A of Poutanen et al. 2014, for more discussion).”
• HIGH-RESOLUTION LINEAR POLARIMETRIC IMAGING FOR THE EVENT HORIZON TELESCOPE (2016, background): “The isotropic total variation TV of a complex image matrix X typically used for image reconstruction and denoising (Rudin et al. 1992) is”
• FIRE-2 simulations: physics versus numerics in galaxy formation (2017, neutral): “…1 + T 0.5 1677.6 )−1.748 αdi = 1.9×10−3 T 1.5 exp ( −470000 T ) × (B14)( 1 + 0.3 exp [ −94000 T ]) Note the αdi term here comes from dielectric recombination. c© 0000 RAS, MNRAS 000, 000–000 (iv) Free-free emission: from Rybicki & Lightman (1986): ΛFF =βff(T ) (ñHI + ñHeI + 4…”
• THE REPEATING FAST RADIO BURST FRB 121102: MULTI-WAVELENGTH OBSERVATIONS AND ADDITIONAL BURSTS (2016, background): “In the optically thin regime, the free-free volume emissivity is given by ν = 5.4 × 10−39T 1/2 e n2eg erg cm −3 s−1 Hz−1 sr−1 (Rybicki & Lightman 1979) for a pure hydrogen plasma, where g is the Gaunt factor, approximately 5.5 for our case.”
• Obscured Active Galactic Nuclei (2018, background): “Physically this is referred to as the optical depth, which is the product of the opacity and density of the material (κλ; ρ) and the path length (s); for example, see Rybicki & Lightman (1979) for a general overview.”
• Dissipative hidden sector dark matter (2014, background): “fˆ(jZ0j 2), where f 1 accounts for partial ionization of the remaining atomic states. 23 Under the assumption that the main source of dissipation is thermal dark bremsstrahlung, ( T) / p T(see e.g. [53]). The temperature Tis related to the rotational velocity of the galaxy far from the center, v 1, ”
• Solar thermophotovoltaics: reshaping the solar spectrum (2016, background): “In other cases, particularly in the far-field, the selective emission property of any structure of a given material can be readily predicted by Kirchhoff’s law of thermal radiation [79], which simplifies the problem of simulating the random nature of thermal emission to that of designing a perfect a”