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20042020
most citedAn Extensive Collection of Stellar Wind X-ray Source Region Emission Line Parameters,Temperatures, Velocities, and Their Radial Distributions as Obtained from Chandra Observations of 17 OB Stars

85 citations · 280 across the 9 of their papers we have counts for

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Showing 2008 · astro-phShow all

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astro-ph2008★ 28 cited

The Effects of Clumps in Explaining X-ray Emission Lines from Hot Stars

J. P. Cassinelli, R. Ignace, W. L. Waldron +3

It is now well established that stellar winds of hot stars are fragmentary and that the X-ray emission from stellar winds has a strong contribution from shocks in winds. Chandra hi…