observed

a r X i v :a s t r o -p h /0411351v 2 26 D e c 2004Mon.Not.R.Astron.Soc.000,1–12(2003)Printed 2February 2008(MN L A T E X style ?le v2.2)

Positron annihilation spectrum from the Galactic Center region observed by SPI/INTEGRAL

E.Churazov,1,2R.Sunyaev,1,2S.Sazonov,1,2M.Revnivtsev,1,2D.Varshalovich,31Max-Planck-Institut f¨u r Astrophysik,Karl-Schwarzschild-Strasse 1,85741Garching,Germany 2Space Research Institute (IKI),Profsoyuznaya 84/32,Moscow 117997,Russia 3Io?e Institute,Polytekhnicheskaya 26,St Petersburg 194021,Russia 2F

Theor.Appl.Climatol.77,39–45(2004)DOI

10.1007/s00704-003-0018-3

40M.Gemmeretal.

1990sandthewatershortageintheYellowrivercatchmentbothofwhichhavebeenaggravatedbyhumanactivities(Kingetal.,2001).Therefore,thedetailedanalysisofprecipitationvariationsareimportantfortheassessmentofclimateinducedrisksandcountermeasures.2.Dataandmethodology

Thedatasetof160NationalMeteorologicalObservatory(NMO)stationswithlong-termmonthlyprecipitationdatainChinahavebeenanalysedinthisstudy.TheyhavebeenprovidedbytheNationalClimaticCentre(NCCC)oftheChinaMe

A self-consistent stellar dynamical model for the Galactic bar is constructed from about 500 numerically computed orbits with an extension of the Schwarzschild technique. The model fits the {\sl COBE} found asymmetric boxy light distribution and the observ

astro-ph/9508146 30 Aug 1995

A self-consistent stellar dynamical model for the Galactic bar is constructed from about 500 numerically computed orbits with an extension of the Schwarzschild technique. The model fits the {\sl COBE} found asymmetric boxy light distribution a

Theor.Appl.Climatol.77,39–45(2004)DOI

10.1007/s00704-003-0018-3

40M.Gemmeretal.

1990sandthewatershortageintheYellowrivercatchmentbothofwhichhavebeenaggravatedbyhumanactivities(Kingetal.,2001).Therefore,thedetailedanalysisofprecipitationvariationsareimportantfortheassessmentofclimateinducedrisksandcountermeasures.2.Dataandmethodology

Thedatasetof160NationalMeteorologicalObservatory(NMO)stationswithlong-termmonthlyprecipitationdatainChinahavebeenanalysedinthisstudy.TheyhavebeenprovidedbytheNationalClimaticCentre(NCCC)oftheChinaMe

We analyze a time series of high angular resolution magnetograms of quiet Sun Inter-Network (IN) magnetic fields. These magnetograms have a spatial resolution better than 0.5 arcsec, a noise of some 20 G, and they have been obtained at the disk center duri

We analyze a time series of high angular resolution magnetograms of quiet Sun Inter-Network (IN) magnetic fields. These magnetograms have a spatial resolution better than 0.5 arcsec, a noise of some 20 G, and they have been obtained at the disk center duri

We analyze a time

Using large number of Rossi X-ray Time Explorer observations of Sco X-1 we present a detailed investigation of the transition layer (TL) and the relativistic precession (RP) models. These models predict the existence of the invariant quantities: an inclina

THEASTROPHYSICALJOURNAL,571:L000,2002JUNE1

APreprinttypesetusingLTEXstyleemulateapjv.11/12/01

CANANY“INVARIANTS”BEREVEALEDINQUASI-PERIODICPHENOMENAOBSERVEDFROM

SCOX-1?

SERGEYKUZNETSOV1

Received2002February25;Accepted2002April19

AND

LEVTITARCHUK2,3

arXiv:astro-ph/0204456v1 26 Apr