71,104 research outputs found
Optical-Near Infrared Color Gradients of Elliptical Galaxies and Their Environmental Dependence
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 r(V)s (half-light radii measured in V-band)
are in general larger than r(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
In this paper we study a question related to the classical Erd\H{o}s-Ko-Rado
theorem, which states that any family of -element subsets of the set in which any two sets intersect, has cardinality at most
.
We say that two non-empty families are are {\it -cross-intersecting}, if for any we have . In this paper we determine the
maximum of for all . This generalizes a result
of Hilton and Milner, who determined the maximum of
for nonempty -cross-intersecting families.Comment: This article was previously a portion of arXiv:1603.00938v1, which
has been spli
Measuring in decays
We develop a method to measure the CKM angle without hadronic
uncertainties from the analysis of and K^\pm \D0bar
followed by singly Cabibbo-suppressed decays to non CP-eigenstates, such as
. This method utilizes the interference between and 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
Recommended from our members
A list of common expressions featuring the postposition ko.
The principal use of ko is to mark an object. In mE# ram ko btaĂĂ
ga âIâll tell Ramâ, ram is said to be the DIRECT
object because the action of telling is done to him directly. In mE# yh tohÂżPa ram ko dUĂ
ga âIâll give this present to
Ramâ, ko means âtoâ and is used to mark the INDIRECT object ram; the direct object is yh tohÂżPa and does not
take ko.
Another use of ko is to pinpoint days of the week or times of day: gu<var ko âon Thursdayâ, subh ko âin the
morningâ, xam ko âin the eveningâ, rat ko âat nightâ (but idn me# âin the daytimeâ).
So much for the primary uses of ko. The purpose of this handout is to list some of the very numerous
constructions and expressions in which ko has a different function. While expressions such as âI have a coldâ
or âI like bananasâ have âIâ as subject in English, in Hindi this âlogical subjectâ takes ko (muJko) and the cold
or the banana becomes the grammatical subject, with which the verb agrees (Âżjukam hE): muJko Âżjkam hE âI have
a coldâ, muJko kele psMd hE# âI like bananasâ.
Each of these expressions can refer to either a male or a female, because the pronoun has no gender. And
muJko can of course be replaced by its synonym muJe.
Familiarise yourself with this list by reading it aloud, and try some substitution exercises by changing the âIâ
to other pronouns and tenses â âShe has a cold, they had a coldâ, etc. Then read the note at the end.Asian Studie
LFV in semileptonic decays and conversion in nuclei in SUSY-seesaw
Here we review the main results of LFV in the semileptonic tau decays (), (), and () as well as in 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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