redback.transient_models.stellar_interaction_models
Functions
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Parameters: :param time: time in source frame in days :param redshift: redshift :param M_star: Mass of the Wolf-Rayet star in solar masses :param M_bh: Mass of the black hole in solar masses :param M_fast: Mass of the fast component in solar masses :param M_pre: Mass of the pre-merger CSM in solar masses :param v_fast: Velocity of the fast component in units of c :param v_slow: Velocity of the slow component in km/s :param alpha: Viscosity parameter :param eta: Efficiency of conversion of accretion energy to radiation :param kwargs: Additional parameters - Must be all the kwargs required by the specific photosphere, sed methods used e.g., for TemperatureFloor: vej (km/s) and temperature_floor :param theta: Disk aspect ratio :param phi_0: Solid angle of the slow component :param kappa_s: Opacity of the slow component :param kappa_f: Opacity of the fast component :param kappa_x: Opacity of the x-ray component :param N: Number of pre-merger orbits :param photosphere: Default is TemperatureFloor. kwargs must have vej or relevant parameters if using different photosphere model :param frequency: Required if output_format is 'flux_density'. frequency to calculate - Must be same length as time array or a single number). :param bands: Required if output_format is 'magnitude' or 'flux'. :param output_format: 'flux_density', 'magnitude', 'spectra', 'flux', 'sncosmo_source' :param lambda_array: Optional argument to set your desired wavelength array (in Angstroms) to evaluate the SED on. :param cosmology: Cosmology to use for luminosity distance calculation. Defaults to Planck18. Must be a astropy.cosmology object. :return: set by output format - 'flux_density', 'magnitude', 'dynamics_output', 'spectra', 'flux', 'sncosmo_source'. |
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Parameters: :param time: time in source frame in days :param M_star: Mass of the Wolf-Rayet star in solar masses :param M_bh: Mass of the black hole in solar masses :param M_fast: Mass of the fast component in solar masses :param M_pre: Mass of the pre-merger CSM in solar masses :param v_fast: Velocity of the fast component in units of c :param v_slow: Velocity of the slow component in km/s :param alpha: Viscosity parameter :param eta: Efficiency of conversion of accretion energy to radiation :param kwargs: Additional parameters :param output_format: whether to output dynamics or bolometric luminosity :param theta: Disk aspect ratio :param phi_0: Solid angle of the slow component :param kappa_s: Opacity of the slow component :param kappa_f: Opacity of the fast component :param kappa_x: Opacity of the x-ray component :param N: Number of pre-merger orbits :return: bolometric luminosity or dynamics output |