Homework Day 8, Sept 21 1) NGC 7027 has a distance of about 920 pc and diameter of about 14 seconds of arc a. How does its diameter compare with its thickness (from previous homework)? Diameter D = θ(radians) × Distance d = 6.7787×10⁻⁵ radians × 920 pc = 0.0624 pc. This is very comparable to the result from HW7 (0.617). Well within 10%. b. Its shell is expanding at about 20km/s. How old is it? (how long ago was the shell ejected?) age t = (0.0624 pc) / (20 km s⁻¹ × 3.24×10⁻¹⁷ pc / 10⁻³ km) × (3.17×10⁻⁸ years / 1.00 s) = 4.50×10⁷ years. 2) The Orion nebula is about 400 pc distant and has an apparent diameter of about 60 minutes of arc. a. What is its physical diameter? D = 6.98 pc. b. The gas density is about 10 4 cm -3 and its temperature is about 10 4 K. The turnover frequency is obvious on Wilson’s SED plot. How thick is the H + layer along our line of sight? turnover ν = 500 MHz. At turnover, τ = 1. Gaunt factor g = 10.6 + 1.9 log(T) - 1.26 log(Z ν) = 7.24. κ′ₛ = 0.178 Z² g ν⁻² T^(-3/2) nₑ nₕ = 5.15×10⁻¹⁶ cm⁻¹. Thickness l = τ / κ′ₛ. 3) The Perseus cluster of galaxies is about 73.6 Mpc distant and has an angular diameter of 860 arc minutes. The total mass in stars is about 2×10 13 M sun and the virial mass is about 10 15 M sun . It is one of the strongest x-ray sources in the sky, with L x = 4x10 45 erg/s. X-rays come from 5 million Kelvin brems. a. Use total luminosity to find the emission measure. L = 4π j V. 4π j = (From AGN3) 1.42×10⁻²⁷ Z² √T g[ff] n². I will adopt an average g[ff] = 1.3. Emission measure n² V = L / (4π 1.42×10⁻²⁷ Z² √T g[ff]) = 7.71×10⁶⁷ cm⁻³. b. Use diameter to find V Spherical V = 4/3 π r³ = 4/3 π (2.84×10²⁵ cm)³ = 9.61×10⁷⁶ cm³. c. Solve for the density n² = 7.71×10⁶⁷ cm⁻³ / 9.61×10⁷⁶ cm³ = 8.03×10⁻¹⁰. n = √n² = 2.83×10⁻⁵ cm⁻³. d. What is the total mass in hot gas? M = μ n V μₕ = 1.67×10⁻²⁷ kg × 2.83×10⁻⁵ cm⁻³ × 9.61×10⁷⁶ cm³ = 2.29×10¹⁵ Mₛₒₗ.