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19932026
most citedParallaxes and proper motions of interstellar masers toward the Cygnus X star-forming complex. I. Membership of the Cygnus X region

329 citations

Showing 2010Show all

16 papers · 1 filter

gr-qc2010

Weyl invariant Dirac-Born-Infeld-Einstein theory

Nahomi Kan, Takuya Maki, Kiyoshi Shiraishi

We consider a Weyl invariant extension of Dirac-Born-Infeld type gravity. An appropriate choice of the metric hides the scalar degree of freedom which is required by the local scal…

astro-ph.GA2010★ 1 cited

A preliminary distance to W 75N in the Cygnus X star-forming region

K. L. J. Rygl, A. Brunthaler, K. M. Menten +6

Cygnus X is one of the closest giant molecular cloud complexes and therefore an extensively studied region of ongoing high mass star formation. However, the distance to this region…

math.AC2010★ 3 cited

Sharp upper bounds of the Betti numbers for a given Hilbert polynomial

Giulio Caviglia, Satoshi Murai

We show that there exists a saturated graded ideal in a standard graded polynomial ring which has the largest total Betti numbers among all saturated graded ideals for a fixed Hilb…

math.CO2010★ 2 cited

Face vectors of simplicial cell decompositions of manifolds

Satoshi Murai

In this paper, we study face vectors of simplicial posets that are the face posets of cell decompositions of topological manifolds without boundary. We characterize all possible fa…

quant-ph2010★ 33 cited

Schrödinger uncertainty relation, Wigner-Yanase-Dyson skew information and metric adjusted correlation measure

Shigeru Furuichi, Kenjiro Yanagi

In this paper, we give a Schrödinger-type uncertainty relation using the Wigner-Yanase-Dyson skew information. In addition, we give Schrödinger-type uncertainty relation by use of…

astro-ph.CO2010★ 7 cited

What Kinds of Accretion Disks Are There in the Nuclei of Radio Galaxies?

Osamu Kaburaki, Takanobu Nankou, Naoya Tamura +1

It seems to be a widely accepted opinion that the types of accretion disks (or flows) generally realized in the nuclei of radio galaxies and in further lower mass-accretion rate nu…