14 research outputs found

    Near-IR period-luminosity relations for pulsating stars in ω\omega Centauri (NGC 5139)

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    ω\omega Centauri (NGC 5139) hosts hundreds of pulsating variable stars of different types, thus representing a treasure trove for studies of their corresponding period-luminosity (PL) relations. Our goal in this study is to obtain the PL relations for RR Lyrae, and SX Phoenicis stars in the field of the cluster, based on high-quality, well-sampled light curves in the near-infrared (IR). ω\omega Centauri was observed using VIRCAM mounted on VISTA. A total of 42 epochs in JJ and 100 epochs in KSK_{\rm S} were obtained, spanning 352 days. Point-spread function photometry was performed using DoPhot and DAOPHOT in the outer and inner regions of the cluster, respectively. Based on the comprehensive catalogue of near-IR light curves thus secured, PL relations were obtained for the different types of pulsators in the cluster, both in the JJ and KSK_{\rm S} bands. This includes the first PL relations in the near-IR for fundamental-mode SX Phoenicis stars. The near-IR magnitudes and periods of Type II Cepheids and RR Lyrae stars were used to derive an updated true distance modulus to the cluster, with a resulting value of (mM)0=13.708±0.035±0.10(m-M)_0 = 13.708 \pm 0.035 \pm 0.10 mag, where the error bars correspond to the adopted statistical and systematic errors, respectively. Adding the errors in quadrature, this is equivalent to a heliocentric distance of 5.52±0.275.52\pm 0.27 kpc.Comment: 10 pages, 8 figures, accepted for publication in A&

    Calibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique I. The p-factor, the Milky Way relations, and a universal K-band relation

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    We determine Period-Luminosity relations for Milky Way Cepheids in the optical and near-IR bands. These relations can be used directly as reference for extra-galactic distance determination to Cepheid populations with solar metallicity, and they form the basis for a direct comparison with relations obtained in exactly the same manner for stars in the Magellanic Clouds, presented in an accompanying paper. In that paper we show that the metallicity effect is very small and consistent with a null effect, particularly in the near-IR bands, and we combine here all 111 Cepheids from the Milky Way, the LMC and SMC to form a best relation. We employ the near-IR surface brightness (IRSB) method to determine direct distances to the individual Cepheids after we have recalibrated the projection factor using the recent parallax measurements to ten Galactic Cepheids and the constraint that Cepheid distances to the LMC should be independent of pulsation period. We confirm our earlier finding that the projection factor for converting radial velocity to pulsational velocity depends quite steeply on pulsation period, p=1.550-0.186*log(P) in disagrement with recent theoretical predictions. We delineate the Cepheid PL relation using 111 Cepheids with direct distances from the IRSB analysis. The relations are by construction in agreement with the recent HST parallax distances to Cepheids and slopes are in excellent agreement with the slopes of apparent magnitudes versus period observed in the LMC.Comment: Accepted for publication by Astronomy and Astrophysics. 15 pages, 11 figure

    Political forgiveness’ transformative potentials

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    The aim of this paper is to contribute to the theoretical and empirical understandings of the role that political forgiveness plays in the post-conflict and post-authoritarian societies. The paper provides a discussion of the complexities of the concept of political forgiveness, and offers empirical examples that demonstrate the different capacities and potentials that political forgiveness has as a mode of social reconciliation and repair the past injustice. It argues that today, with the accumulation of experience in the practice of transitional justice, and the growing importance of human rights regime, considering of forgiveness through the accountability’s lens is very timely and important. After the discussion of the contribution of forgiveness to societal reconstruction in the post-conflict and post-authoritarian societies, the paper focuses on the role of forgiveness as an essential part of justice and solidarity. By scrutinizing forgiveness’ links with reconciliation and justice, the paper offers a comprehensive way to assess the nature of preconditions and the role of forgiveness in addressing the past injustice and overcoming divisions in post-conflict societies. Its discussion of empirical findings on the role that forgiveness opens up a debate about risks and costs involved in a policy of forgiveness in newly democratized countries
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