The Normative Agency of Regional Organizations and Non‐governmental Organizations in International Peace Mediation

This article analyzes the increasingly prominent role of regional organizations (ROs) and non‐governmental organizations (NGOs) in promoting norms in mediation processes. In particular, we seek to understand the processes by which RO and NGO mediators promote the inclusivity norm to negotiating parties and the outcomes that result. We employ the concepts of local agency and social practices in examining the normative agency of ROs and NGOs in promoting and redefining the inclusivity norm. Through illustrative case studies of peace processes in South Sudan and Myanmar, we argue that ROs’ and NGOs’ mediation practices reflect their claims to alternative resources of power, such as long‐standing expertise and insider status in the context, and build congruence with strong local norms. We provide nuanced theoretical insights on RO and NGO mediators’ claims to agency and provide empirical illustrations on how these claims contribute to constitutive changes to norms

Horizontal Branch Stars: The Interplay between Observations and Theory, and Insights into the Formation of the Galaxy

We review HB stars in a broad astrophysical context, including both variable and non-variable stars. A reassessment of the Oosterhoff dichotomy is presented, which provides unprecedented detail regarding its origin and systematics. We show that the Oosterhoff dichotomy and the distribution of globular clusters (GCs) in the HB morphology-metallicity plane both exclude, with high statistical significance, the possibility that the Galactic halo may have formed from the accretion of dwarf galaxies resembling present-day Milky Way satellites such as Fornax, Sagittarius, and the LMC. A rediscussion of the second-parameter problem is presented. A technique is proposed to estimate the HB types of extragalactic GCs on the basis of integrated far-UV photometry. The relationship between the absolute V magnitude of the HB at the RR Lyrae level and metallicity, as obtained on the basis of trigonometric parallax measurements for the star RR Lyrae, is also revisited, giving a distance modulus to the LMC of (m-M)_0 = 18.44+/-0.11. RR Lyrae period change rates are studied. Finally, the conductive opacities used in evolutionary calculations of low-mass stars are investigated. [ABRIDGED]Comment: 56 pages, 22 figures. Invited review, to appear in Astrophysics and Space Scienc