Physics of the Interstellar and Intergalactic Medium

By B. Draine. 2011

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View Paper: https://www.semanticscholar.org/paper/4044da71198b1fdfd7eaeb2848ec2ee656d4db39

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In Astronomy and Astrophysics

Citations in the corpus

Planck intermediate results: XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds (2015, neutral): “The X CO factor may show cloud-to-cloud or regional variations (Draine 2011), but we consider that these are not signiﬁcant in comparison to the uncertainties involved in the estimation of B ⊥ .”
Toward an understanding of foreground emission in the BICEP2 region (2014, neutral): “perpendicular to the starlight polarization direction [37].”
How to Calculate Molecular Column Density (2015, methodology): “…radiative transfer equation, ignoring scattering processes (such as those involving electrons or dust) is defined as follows (see Spitzer (1978) or Draine (2011) for details): dIν ds = −κνIν + jν (12) where s ≡ Path of propagation along the line of sight Iν ≡ Specific Intensity κν ≡ Absorption…”
An origin for multiphase gas in galactic winds and haloes (2015, background): “…large distance as a result of adiabatic cooling, the shape of the cooling function changes, and can be approximated as (e.g., Mac Low & McCray 1988; Draine 2011) Λ(T ) = ε̇/n2 ' 3× 10−23 T−0.77 ξ (10 5 ∼< T ∼< 10 7 K), (1) where T7 = T/107 K and where ξ is meant to capture the dependence of Λ on…”
Star Formation in the Milky Way and Nearby Galaxies (2012, background): “8.11 in Draine 2011).”
The SILCC (SImulating the LifeCycle of molecular Clouds) project - II. Dynamical evolution of the supernova-driven ISM and the launching of outflows (2015, methodology): “To compute the Hα fluxes we follow the same procedure as outlined in Gatto et al. (2015) accounting for collisional excitation and radiative recombination of ionized hydrogen (Dong & Draine 2011; Draine 2011; Kim et al. 2013).”
Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics (2017, background): “3 10 100 Ke 9 1 2cm3 s−1, and sá ñ » ´v 2.0i -10 9cm3 s−1 are coefficients of momentum exchange in electron-neutral and ion-neutral collisions (Draine 2011).”
HERSCHEL SURVEY OF GALACTIC OH+, H2O+, AND H3O+: PROBING THE MOLECULAR HYDROGEN FRACTION AND COSMIC-RAY IONIZATION RATE (2014, positive): “A prescription for calculating the steady-state value of xe as a function of ζH in purely atomic gas is given by Draine (2011), and includes the effects of grain-assisted recombination (Weingartner & Draine 2001).”
Thanatology in protoplanetary discs - The combined influence of Ohmic, Hall, and ambipolar diffusion on dead zones (2014, background): “is the ion-neutral collision rate (Draine 2011); mn and mi are the average masses of the neutrals and ions, respectively.”
H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations (2017, background): “Further information about dust grains and their laboraory analogs can be found in Draine (2011) , Henning (2010a, b) , ones et al. (2013) , Krügel (2007) .”
THE CO-TO-H2 CONVERSION FACTOR AND DUST-TO-GAS RATIO ON KILOPARSEC SCALES IN NEARBY GALAXIES (2012, positive): “Following the derivation in Draine (2011), αCO = 3.4n 0.5 3 (e 5.5/Tex−1) M pc−2(K km s−1)−1.”
A BUDGET AND ACCOUNTING OF METALS AT z ∼ 0: RESULTS FROM THE COS-HALOS SURVEY (2013, background): “…the Weingartner & Draine (2001), Zubko et al. (2004), and Draine & Fraisse (2009) dust models to constrain the oxygen fraction of dust (see also Draine 2011), we find Moxy,dust Mdust = µoxyN oxy dust ∑ X µXNXdust , (A2) where µ is the average atomic mass, X is one of the elements C, N, O, Mg,…”
The Critical Density and the Effective Excitation Density of Commonly Observed Molecular Dense Gas Tracers (2015, neutral): “– 8 – as uνjk = uνjk(Tbg)β̄ + uνjk(Tex)(1 − β̄) , (7) where β̄ is the solid angle averaged escape fraction (see Chapter 19 of Draine 2011 for a derivation).”
Physical Processes in the Interstellar Medium (2014, methodology): “This general behavior remains true in more recent models (see the detailed discussion by Draine, 2011).”
THE 2013 RELEASE OF CLOUDY (2013, background): “Texts that review this field include Spitzer (1978), Dopita & Sutherland (2003), Tielens (2005), Osterbrock & Ferland (2006) (hereafter AGN3), and Draine (2011).”
The big problems in star formation: The star formation rate, stellar clustering, and the initial mass function (2014, background): “The unattenuated ISRF of the Milky Way carries an energy density ≈ 6− 9× 10−14 erg cm−3 integrated over the energy range 6−13.6 eV (Draine 1978; Mathis et al. 1983; Draine 2011).”