71,104 research outputs found

    Optical-Near Infrared Color Gradients of Elliptical Galaxies and Their Environmental Dependence

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    We have studied the environmental effect on optical-NIR color gradients of 273 nearby elliptical galaxies. Color gradient is a good tool to study the evolutionary history of elliptical galaxies, since the steepness of the color gradient reflects merging history of early types. When an elliptical galaxy goes through many merging events, the color gradient can be get less steep or reversed due to mixing of stars. One simple way to measure color gradient is to compare half-light radii in different bands. We have compared the optical and near infrared half-light radii of 273 early-type galaxies from Pahre(1999). Not surprisingly, we find that re_{e}(V)s (half-light radii measured in V-band) are in general larger than re_{e}(K)s (half-light radii measured in K-band). However, when divided into different environments, we find that elliptical galaxies in the denser environment have gentler color gradients than those in the less dense environment. Our finding suggests that elliptical galaxies in the dense environment have undergone many merging events and the mixing of stars through the merging have created the gentle color gradients.Comment: 3 pages, 2 figures. Proceedings of the 6th East Asian Meeting of Astronomy, held at Seoul National University, Korea, from October 18-22, 200

    Uniform s-cross-intersecting families

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    In this paper we study a question related to the classical Erd\H{o}s-Ko-Rado theorem, which states that any family of kk-element subsets of the set [n]={1,
,n}[n] = \{1,\ldots,n\} in which any two sets intersect, has cardinality at most (n−1k−1){n-1\choose k-1}. We say that two non-empty families are A,B⊂([n]k)\mathcal A, \mathcal B\subset {[n]\choose k} are {\it ss-cross-intersecting}, if for any A∈A,B∈BA\in\mathcal A,B\in \mathcal B we have ∣A∩BâˆŁâ‰„s|A\cap B|\ge s. In this paper we determine the maximum of ∣A∣+∣B∣|\mathcal A|+|\mathcal B| for all nn. This generalizes a result of Hilton and Milner, who determined the maximum of ∣A∣+∣B∣|\mathcal A|+|\mathcal B| for nonempty 11-cross-intersecting families.Comment: This article was previously a portion of arXiv:1603.00938v1, which has been spli

    Measuring Îł\gamma in B±→K±(KK∗)DB^\pm \to K^\pm (K K^*)_D decays

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    We develop a method to measure the CKM angle Îł\gamma without hadronic uncertainties from the analysis of B±→K±D0B^\pm \to K^\pm D^0 and K^\pm \D0bar followed by singly Cabibbo-suppressed DD decays to non CP-eigenstates, such as K±K∗∓K^\pm K^{*\mp}. This method utilizes the interference between b→cuˉsb\to c\bar u s and b→ucˉsb\to u\bar c s decays, and we point out several attractive features of it. All the modes that need to be measured for this method are accessible in the present data.Comment: 8 page

    LFV in semileptonic τ\tau decays and Ό−e\mu-e conversion in nuclei in SUSY-seesaw

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    Here we review the main results of LFV in the semileptonic tau decays τ→ΌPP\tau \to \mu PP (PP=π+π−,π0π0,K+K−,K0Kˉ0PP = \pi^+ \pi^-, \pi^0 \pi^0, K^+ K^-, K^0 \bar{K}^0), τ→ΌP\tau \to \mu P (P=π,η,ηâ€ČP = \pi, \eta, \eta^{\prime}), and τ→ΌV\tau \to \mu V (V=ρ,ϕV = \rho, \phi) as well as in Ό−e\mu-e conversion in nuclei within SUSY-seesaw scenarios, and compare our predictions with the present experimental boundsComment: Talk given by M. J. Herrero in SUSY08 conference, Seou
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