The Sony Xperia Z is one of the most eagerly awaited smartphones of 2013 and that might be because of its latest UI. You can use this post to learn how to install the Sony Xperia Z Launcher using a simple APK file, and get the latest features of the Xperia Z user interface
right for your Android device.
The APK of the Sony Xperia Z official launcher can be installed on any Android 4.0.3 and later smartphones. Below you can find a list of its most important features:
it can be installed on any Android device with any resolution and DPI setings.
user selectable desktop and app drawer grid size up to 12×12.
support for assigning swipe, pinch and double tap gestures
infinite scrolling
it works with Launcher Pro and Go Launchers icon packs
you can customize individual shortcuts by setting icons and label
backup and restore support for backing up launcher data
you can add shortcuts for launcher actions and any other activity
you can search for apps right from the app drawer
you can create folders in the app drawer only when using the ‘own order’ function instead of ‘alphabetical’, ‘most used’ or ‘recently installed’ options.
works with Android 4.0.3 and later variants.
in the next days you should see that widget addition will be supported, too.
There are tons of other features that you can experience only by installing this launcher. In order to make sure that you successfully install the Sony Xperia Z Home Launcher APK on your device, you should take a look at the guidelines listed below, too.
Sony Xperia Z custom launcher APK for all the other Android 4.0.3 and later smartphones has been created and released by ‘ra3al’, an XDA member and developer. Here’s what you need to know in order to make sure that you’re device can support the installation of this new custom launcher:
Obviously, your device should be on Android 4.0.3 ICS or any other later build.
You should have a backup of the settings of your current launcher, just in case something goes wrong and you lose its setup after the new launcher is installed.
Go to Settings menu, open ‘Security’ and enable the option that says ‘Unknown sources’.
This will allow you to flash new custom APKs directly from your device’s SDcard.
You need to have installed a file managing application so that you will be able to find the APK file.
now that you know all of the above, you can install the new launcher.
Here’s how to install Sony Xperia Z Launcher APK on your Android 4.0.3+ smartphones:
Download the APK of the Xperia Z launcher from HERE.
You can save your file on your computer and move it to your smartphone after the download is complete or, you can download it directly to your phone.
Open the File Manager app and browse your phone’s folders to find the Xperia Z APK file. For Jelly Bean devices you can tap once the Xperia Z Launcher APK download complete notification and confirm the installation.
Confirm that you want to install the new Xperia Launcher.
Tap on the Home button of your phone and select Xperia Launcher to launch this new custom launcher app.
Customize the home screen and all the other menus for it suit your needs.
These were all the steps that you had to take and now you’re free to test the new launcher. If you find any bugs or errors when testing Xperia Z Launcher, then you can tell us in comments or you can choose to visit the
for this custom APK. If you cannot complete the installation then you can ask for extra help by leaving a detailed comment at the end of this post.应用程序华为桌面（进程com.huawei laun cher3）意外停止_百度知道
应用程序华为桌面（进程com.huawei laun cher3）意外停止
应用程序华为桌面（进程com.huaweilaun cher3）意外停止
两个方法：一，进入应用程序，找到华为桌面清除数据，如果不行。连接豌豆荚，安装一个第三方桌面，然后启动进入第三方桌面，把第三方桌面设置默认，停用或者卸载之前的出问题的桌面。二，网上下载一个官方ROM，提取里面的华为桌面APK，安装替换进去。或者重刷和你现在系统一样的ROM，最好备份资料，当然刷别的ROM也行。看你自己选择！连接豌豆荚可以备份短信和通讯录。PS：除了豌豆荚，还有91助手，其他助手等。本人习惯豌豆荚所以上面举例豌豆荚！
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出门在外也不愁eclipse executable launcher was unable to locate its companion shared library.
i had delete my eclipse and Sdk also because they did not generate R.java file so i think delete the eclipse and then extract the
eclipse zip after extract the zip then i click it show that error
"eclipse executable launcher was unable to locate its companion shared library".How to solve
this problem . i read the many article but did not find the best solution .My laptop configuration is dual core 3 gb ram 320 hd ,32bit .
Unzip again. Make sure that your unzip tool extracts directories. This error is typical for unzipping to a flat folder structure.
14.6k43257
Happened to me too, because I tried to run the eclipse before the unzip process has finished.
Make sure that the unzip process has finished.
18.3k21947
You might want to check that library
org.eclipse.equinox.launcher_.dist.jar
plugins/org.eclipse.equinox.launcher.gtk.linux.x86_.dist
exists on your system.
Make sure that the version of libraries mentioned in eclipse.ini and the version that exists on your system is same. Usually after upgrade this mismatch occurs and eclipse fails to locate the required jar.
Please take a look at this blog post
In eclipse.ini, I noticed some paths contained dashes, which denote a new arguement.
It is a simple fix:
plugins/org.eclipse.equinox.launcher_1.3.0.v8.jar
--launcher.library
plugins/org.eclipse.equinox.launcher.win32.win32.x86_64_1.1.200.v6
plugins/org.eclipse.equinox.launcher_1.3.0.v.jar
--launcher.library
plugins/org.eclipse.equinox.launcher.win32.win32.x86_64_1.1.200.v
But, you must also do the same to the actual files.
Hope this helps!
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Stack Overflow works best with JavaScript enabled79The Molecular Gas Environment around Two Herbig AeBe Stars Resolving the Outflows of LkHa 1-第3页
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79The Molecular Gas Environment around Two Herbig AeBe Stars Resolving the Outflows of LkHa 1-3
Out?owsfromHerbigAe/BeSt；11；Fig.8.―Position-velocity；clearlyrevealsthepresenc；COJ=2?1emissiondetectedb；Figures5and6providefurth；Figure8showstheP?Vdiagra；taposedonthezerothmoment；4.
Out?owsfromHerbigAe/BeStars11Fig.8.―Position-velocitydiagramstakenthroughthetwobluefeaturesmarkedAandBinFigure5areshownalignedthroughboththeLkHα225SandLkHα225Nsources.Itisnotpossibletodiscriminatewhetherfeature“A”arisesfromLkHα225SorLkHα225N.FeatureBshowsvirtuallythesamepro?lethroughbothsources.Sincethisfeatureisalignedwiththeo?setbetweenthesources,discriminationisnaturallydi?cult.Thereisstillsomeevidenceforthepole-onout?owofLkHα225S(seeFig.7)inslicesthroughLkHα225N.clearlyrevealsthepresenceofemissionatthe0′′o?setacrossbothredandblue-shiftedvelocities(from0to20kms?1)withrespecttothesource.TheP?VdiagramproducesthisfeaturenomatterwhattheorientationoftheslicecenteredonLkHα225S.Weinterpretthisemis-sionasarisingfromanout?owdrivenfromLkHα225Sbutobservedalmostpole-on.Thisisconsistentwiththe12COJ=2?1emissiondetectedbyPallaetal.(1995)inwhichthey?ndstronglyoverlappingblueandredlobesinthesingledetectedout?ow.Theblue-shiftedemissioniso?setslightlytotheeastcomparedtotheredlobe,whichisalsoconsistentwiththeplane-of-skyemissionshowninFigure5,butisintheoppositesensetotheout?owlobesobservedbyPallaetal.(1995).Figures5and6providefurtherclari?cationinidentify-ingthedrivingsourcesoftheout?owswithcomponentsintheplaneofthesky.Inadditiontothepole-onout-?ow,asecondout?owappearswell-centeredonLkHα225,basedonthebluelobeofemissiondetectedsouth-eastofthetwosourcesatapositionangleof～145?(EofN).Anotherbluepeakisdetectedtothenortheastoftheclusterofsources(at～45?),suggestingathirdout?owispresentinthesystem.Thereisnoevidenceofcoherenceintheblue-shiftedemissionpeakstosuggesttheyarepartofalarger,blue-shiftedcounterparttothered-shifted“ring”,i.e.,partofthesameout?ow.Figure8showstheP?Vdiagramsacrosstwopo-sitionanglessuggestedbytheorientationoftheblue-shiftedemissiondetectedinthezerothmomentandchan-nelmaps(labeled“A”and“B”inFig.5).Alongtheseslices,thereisevidenceforred-shiftedcomponentscom-plementarytotheblue-shiftedemission.Thered-shiftedemissionfromthesetwopotentialout?owsappearsjux-taposedonthezerothmomentmapofFigure5,lyingcoincidentwiththered-shiftedgasfromthepole-onout-?owandcreatingaringstructurewhichpersistsoverarangeofvelocities,althoughthisemissionappearssignif-icantlyclosertothedrivingsourcesthanthebluelobes.4.1.2.SpectraUsingFCRAO,wehavedetected12COJ=1?0,13COJ=1?0,CSJ=2?1andN2H+J=1?0emissionfromtheLkHα225Sregion.The12COJ=1?0,13COJ=1?0andCSJ=2?1spectraallindicatemultipleemissionpeaksalongthelineofsightandareshownto-wardeachofthefoursourcesinFigure9.Wealsoshowthecombined12COJ=1?0spectraathighspatialandspectralresolution.WeshowanN2H+J=1?0spectrumtowardLkHα225SinFigure10.Strongevi-denceforout?owinggasisdetectedtowardLkHα225SandLkHα225N,butnoneisdetectedtowardBD+404124andonlyevidenceforred-shiftedemissionisseenatthepositionofLkHα224.Weinterpretthehighveloc-ityemissiontowardLkHα224asarisingfromtheout-?owsgeneratedbytheLkHα225sources.LessambientCOappearstobepresentinthisregioncomparedtotheenvironmentaroundLkHα198,sincenosigni?cantself-absorptionisobservedtowardanyofthesourcesinFigure9.Interpretationofthesespectraisfurthercom-plicatedbythepresenceofmultiplecloudsalongthelineofsight.Peaksareobservedat?vedi?erentvelocitiesinthespectra(1.6,3.2,7.9,12.8and14.5kms?1asidenti?edbyeyeinFigure9).Theprimarycloud,at7.9kms?1,appearstocontainalltheHAeBestars.Asec-ondcloud,at12.8kms?1,appearstocontainsigni?cantamountsof12COJ=1?0and13COJ=1?0,butno12Matthewsetal.Fig.9.―SpectratowardindividualsourcesintheLkHα225Sregionresolutionfrom12fromCOJ=isFCRAOandFCRAO+BIMAarraydata.Thespectral1?0.2540,13kmCOs?1J=.Grey,1?0andredandCSJblue=2spectra?1observationsrepresentscalesFCRAOscale13atofwhichwereregriddedtothespatialandspectrallefttheisFCRAO+BIMA12forthesingledishCO12JCO=J1?0map.TheintensitybyCOJ=1?0andCSJ=2?1emission=have1?0emission.Thethefactorsatcombinedoftwo12COandJtwenty.=1?0TheblackspectrabeenaretakenmultipliedfromCygnusright.LkHdoUnlikenotexhibitthesourcesinmap.theTheLkHintensityα198region,scaleisthoseshownindoesαhighnot225Nshowshowanythesigni?cantself-absorption.LkHα225Sandevidencemostextensivelinewings.BD+404124wingsvelocityThewhichcouldblue-shiftedofout?owwhileLkHα224showsnobeassociatedemission,withbutextensivered-shiftedlines?1ofsight..linesThesebelowpeakstheeachplotsrepresentindicateindividual1.6,another3.2,7.9,sourceclouds12.8alongandinthe14.5?eld.thelinekmFig.10.―SpectrumofN2H+J=1?0emissiontowardLkHα225S,indicatingthepresenceofdensegas.CSJ=2?1wasdetectedatthisvelocity.Theevidenceforcloudsattheremainingvelocitiesisbasedon12COJ=1?0only.TheresolutionofFCRAOissuchthatwecannotbesurethatallfoursourcesareassociatedwithdensegas.Asthemostembeddedobject,LkHα225Sisthemostlikelysourcetobeassociatedwithdensegas.How-ever,BD+404124,whichisthefurthestremovedfromLkHα225S,liesonlyabout45′′distant.ThisisonlyoneFCRAObeamwidthatthefrequencyofthe13COJ=1?0emission,andsubstantiallylessthanabeamwidthinCSJ=2?1andN2H+J=1?0.Higherresolutionob-servationscanisolatetheconcentrationsofthesespeciesandenablekinematicstudyoftheassociatedcores.4.1.3.2.6mmContinuumNosign?ciantcontinuumwasdetectedtowardanyofthesourcesinthe?eldcontainingLkHα225S.Oursensi-tivityisratherlow,giventhelimitedbandwidthavailableforcontinuumobservations.Wecanputanupperlimitof51mJybeam?1onthecontinuum?uxoncompactsourcesintheregion.DespitethestrongCOandNJ=1?0detections,weseeno?uxtoattributetoeither2H+dustcontinuumorfree-freeemission.DiFrancescoetal.(1997)detected2.7mmemissionfromLkHα225SusingthePlateaudeBureinterferometerwitharesolutionof6.8′′×14.6′′.Theydetectedapeak?uxdensityof23mJybeam?andatotal?uxdensityof24±6.7mJy.This?uxwouldnothavebeendetectable1ata2σlevelwiththesensitivity(σ=17mJybeam?rms)inourmap.4.2.IndividualSourcesTable5summarizesour?ndingsregarding12COJ=1?0andout?owsinthisregion.Self-absorptionisnotdetectedtowardanysourcesinthis?eld.However,wedodetecttracersofdensegas,including13COJ=1?0,CSJ=2?1andN2H+J=1?0inthiscloud.Wenotealsothatourinterpretationsofout?owsfromLkHα225SandLkHα225Narestillresolution-limited.Therefore,wediscussthesesourcestogetherbelow.4.2.1.LkHα225SandLkHα225NLkHα225Sisfoundtohaveevidenceforuptothreeassociatedout?ows.Themostde?nitiveconnectionisbasedonevidenceforanearlypole-onout?owclearlyseenintheP?VdiagramofFigure7.Evidencefortwoadditionalout?owsisseeninFigure5intheformoftwoblue-shiftedemissionfeatures.Thesolidlinesshowtheaxesformedbythefeatures,“A”and“B”,withLkHα225Sandbothaxesalignwithred-shiftedfeaturesseenontheothersideofthepotentialdrivingsource.How-ever,LkHα225SisseparatedfromLkHα225Nbyonly5′′,whichiscomparabletothemajoraxisofoursynthe-sizedbeam(naturally-weighted).Thismakesitdi?culttoassociatedecisivelyeitherofthesetwoplane-of-skyout?owswithLkHα225S.Basedonalignment,astrongcasecanbemadethatLkHα225Nisdrivingoneorbothoftheseout?ows(seethedashedlinesofFigure5).WeassertthattheapparentringofFigure5hascoher-entstructure,asitisdominatedbythered-shiftedemis-sionofthepole-onout?owwithcontributionsfromtheotherout?owsoriginatingfromtheLkHα225sources,oneorientedatapproximately45-55?EofN,thesecondatabout145-160?EofNandthethirdalmostpole-onto-wardus.Noevidenceoftheringmorphologyisobservedinpreviousdetectionsofhigh-velocitygasintheregion(e.g.,Pallaetal.1995)withresolutiononlyafactorofthreepoorerthanourdata.Aswenotedabove,theinterpretationoftheringasthered-shiftedcounterpartstothemorede?nitivebluelobesontheplaneoftheskysuggeststhattheredlobeshavenotexpandedtothesamespatialextent.TherecentworkofLooneyetal.(2006)suggestsapotentialexpla-nation.TheirhighresolutionBIMAarrayobservationsOut?owsfromHerbigAe/BeStarsTABLE5LkHα225S&SurroundingObjectsSourceLkHα225SLkHα225NBD+404124LkHα224OtherIDV1318SCygV1318NCygV1685CygV1686CygRA(J:30.620:20:30.620:20:28..26DEC(J:25.5+41:21:30.5+41:21:51.6+41:21:28.6Groupa......IIAssociatedCOyesmaybeyesyes#AssociatedOut?ows1-3b0-2bnonenonePA(?EofN)l.o.s.c,45?,145?55?,160?CC13Note.―aClassi?cationofHillenbrandetal.(1992).bThedrivingsourceoftwoout?owscannotbeuniquelyidenti?edasLkHα225SorLkHα225Nduetoremainingresolutionlimitations.cline-of-sight.Theout?owisalmostpole-on,withlittlecomponentintheplaneofthesky.ofCSJ=2?1showthattheCSJ=2?1tracesoutadense?lamentofemissiontothenorthwestoftheLkHα225sources.Thepresenceofdensergasinthisdirectionmaybeimpedingthered-shiftedcomponentoftheout-?owfromextendingintothecloudalongthesepositionangles.4.2.2.BD+404124BD+404124isaGroupIHAeBestarasclassi?edbyHillenbrandetal.(1992).Thismeansthatthereisnoremainingcircumstellaremissionwhichcannotbeac-countedforbyadisk.12COJ=1?0,13COJ=1?0andCSJ=2?1arealldetectedtowardBD+404124basedonthespectraofFigure9.ThisemissionislikelyassociatedwiththeambientmolecularcloudsalongthelineofsighttoCygnus.Thelackofself-absorptionindi-catesthatrelativelylittlegasremainsaroundthissource,andthereisnosigni?cantevidenceoflinewingsinthespectra.4.2.3.LkHα224LkHα224isalsoclassi?edasaGroupIHAeBestarbyHillenbrandetal.(1992).ThespectrumofLkHα224isdominatedbythemultiplepeaksassociatedwithcloudemissionalongthelineofsight.Thecombined12COJ=1?0spectrumdoesshowevidenceofared-shiftedlinewinghowever.Noout?owemissionappearsfocussedonthissourcebasedonthechannelmapsofFigure6,andnoblue-shiftedemissionisinthevicinityofthissourceinthezerothmomentmapofFigure5.Givenitspositionrelativetotheblue-shiftedemissionpeaks,wesurmisethatthered-shiftedemissionobservedatthepositionofthissourceispartofoneoftheout?owsoriginatingfromtheLkHα225sources.5.CONCLUSIONSWe?ndthatthesinglebipolarout?owdetectedintheLkHα198regioninsingle-dishmapsisacombinationofthered-shiftedemissionoftheLkHα198andLkHα198-mmout?owsandtheblue-shiftedcomponentsoftheout?owsfromLkHα198-mmandV376Cas.Inall,we?ndevidenceforfourout?owsintheLkHα198regionusinghigh-resolution12COJ=1?0observations.Ev-idenceforacavityisobservedintheLkHα198systemalongthesameaxisastheellipticalcavitydetectedinopticalandIRemission.Weseenoevidenceforcircum-stellarmaterialbasedon12COJ=1?0emissionas-sociatedwithLkHα198-IR,contrarytotheresultsfromnear-IRpolarimetrywhichassociatedustemissionwiththatsource(Perrinetal.2004a)andobservationsofHHobjects,whichidenti?edLkHα198-IRasadrivingsource(Corcoranetal.1995).Ourabilitytodiscriminatebetweendetected12COJ=1?0out?owsandmeasureindependentmassesandmomentumislimitedbythesinglepointingoftheBIMAarraymaps(Figure3clearlyshowsthatwehavenotmappedtheout?owsintheirentirety)andspatialreso-lution.Theout?owemissionisstillentangledandthecloudemissionisalsoacontaminant.Ideally,mosaickedobservationswithvariousarraycon?gurations(includ-ingveryclosebaselines)willbeobtainedtomaximizethedetectionoftheout?owemission,butminimizethedetection12ofemissionfromtheambientcloud.TheCOJ=1?0emissionfromLkHα225Sisequallycomplex.Inall,we?ndevidenceforuptothreeout?owsinthisregion,alloriginatingfromtheLkHα225sources.Large-scalecloudemissiondominatesthe?eld,andmultiplecloudsalongthelineofsightcontaminatethespectra.Oneisde?nitivelyassociatedwithLkHα225Sandisalmostentirelyalongthelineofsight.Theotherout?owslieatanglesof35?and135?eastofnorthprojectedontotheplaneofthesky.Wesuggestthattheringofred-shiftedemissionisinfactajuxtaposi-tionofthered-shiftedlobesofthesetwoout?ows,wheretheirexpansionhasbeenhinderedduetoadensemolec-ularcloudlyingtothenorthwest,withthecavityofthepole-onout?ow(acoherentstructure).AsintheLkHα198region,higherresolution,mosaickedmapswouldhelpdisentangletheout?owsfromtheLkHα225sources.Estimationofthemassintheseout?owsisnoteasybasedonthedatapresentedherebecausetheycanonlyberesolvedwithintheBIMAarrayantenna?eldofview,whereastheout?owscertainlyextendtolargerspatialscales.Inseveralcases,emissionfromseveralout?owsisclearlycombined,furthercomplicatingtheindependentassessmentsofmasses.Finally,we?ndevidenceofhigherdensitygasinbothregions,with13COJ=1?0andCSJ=2?1detectedtowardalleightsourcesandN2H+J=1?0detectedintheobjectsinCygnus.Localizingtheprecisesourcesofthisemissionrequireshigherresolutionobservations,sincetheseparationofsourcesiscomparableorsmallerthantheFCRAObeam.TheauthorswouldliketothankMarkHeyerforadviceandobservingtheFCRAOdataforus.WethankJ.DiFrancescoforusefuldiscussionsandacarefulreadingofthemanuscript.BCM’sresearchwassupportedbyanNSERCPDFandBerkeleyNSFgrantAST02-28963.MDPwassupportedbyaNASAMichelsonFellowship.14Matthewsetal.theNationalScienceFoundationScienceandTechnologyCenterforAdaptiveOptics,managedbytheUniversityofCaliforniaatSantaCruzundercooperativeagreementNo.AST-9876783.TheBIMAarraywasoperatedwithsupportfromtheNa-tionalScienceFoundationundergrantsAST-02-28963toUCBerkeley,AST-02-28953toU.Illinois,andAST-02-28974toU.Maryland.FCRAOwassupportedbyNSFGrantAST02-28993.ThisworkhasbeensupportedbyREFERENCESArce,H.G.andSargent,A.I.2006,ApJ,646,1070Aspin,C.,Sandell,G.,&Weintraub,D.A.1994,A&A,282,L25Bally,Buisson,J.,&G.,Lada,Desbats,C.J.1983,L.,Duvert,ApJ,265,G.,824Forveille,T.,Gras,R.,Guilloteau,S.,Lucas,R.,&Valiron,P.2002,ContinuumandLinehttp://iram.fr/GS/class/class.htmlAnalysisSingle-DishSystemManual(IRAM:Grenoble),Cant′Caselli,o,Rodr′P.,Benson,?guez,Calvet,P.,Myers,&LevreaultP.,&Tafalla,1984,ApJ,M.ApJ,572,238Caselli,Chavarr′P.,?a-K.,Myers,C.1985,P.C.,A&A,&Thaddeus,148,317P.1995,ApJ,455,L77Chrysostomou,A.,etal.2005,ProtostarsandPlanetsV,8156Corcoran,Corcoran,M.,D.,Ray,&Ray,T.P.,T.&P.Bastien,1998,A&A,P.,A&A,535293,550Davies,R.I.,etal.2001,ApJ,552,692DiDiFrancesco,Francesco,J.,J.,Andr′Evans,e,P.,N.J.,&Myers,II.,Harvey,P.C.2004,P.M.,ApJ,Mundy,617,425L.G.,Dore,Guilloteau,L.,Caselli,S.,&P.,Chandler,Beninati,C.J.S.,1997,Bourke,ApJ,T.,482,Myers,433P.C.,&Cazzoli,G.2003,A&A,413,1177Finkenzeller,Forveille,T.,U.Guilloteau,1985,A&A,S.,151,&Lucas,340R.1989,CLASSManual(Grenoble:IRAM)Fuente,R.,&A.,Neri,Rodr′R.?guez-Franco,2003,A&A?A.,Testi,L.,Natta,A.,Bachiller,Graham,J.R.,Wright,G.S.,&Longmore,A.J.1987,ApJ,313,Hajjar,847R.,&Bastien,P.2000,ApJ,531,494Herbig,Henning,G.Th.,1960,Burkert,ApJS,4,337A.,Launhardt,P.,Leinert,Ch.,&Stecklum,B.1998,A&A,336,565Hern′Hillenbrand,andez,J.,L.A.,etal.Strom,2004,S.E.,AJ,127,Vrba,1682F.J.,&Keene,J.1992,ApJ,397,613Koresko,Lagage,P.O.,C.D.Olofsson,etal.1997,G.,ApJ,Cabrit,485,S.,213Cesarsky,C.J.,Nordh,L.,&RodriguezEspinosa,J.M.1993,ApJ,417,L79Leinert,Looney,Ch.,L.W.,Haas,Wang,M.,S.,&Hamidouche,Lenzen,R.1991,M.,A&A,Sa?er,246,P.N.,180&Klein,R.2006,ApJ,642,330Lynds,Matzner,B.T.,C.D.,1969,&McKee,PASP,81,C.496F.2000,ApJ,545,364McGroarty,F.,Ray,T.P.,&Bally,J.2004,A&A,415,189McGroarty,F.,&Ray,T.P.2004,A&A,420,975Meuus,Mundt,G.,R.&etRay,al.2001,T.P.A&A,,ASP476Conf.Ser.62,237Nakano,M.,Kogure,T.,Yoshida,S.,&Tatematsu,K.1990,PASJ,Natta,42,567A.,Palla,F.,Butner,H.,Evans,N.J.II,&Harvey,P.M.Palla,1992,F.,ApJ,Testi,391,L.,805Hunter,T.R.,Taylor,G.B.,Prusti,T.,Felli,M.,Natta,A.,&Stanga,R.M.1995,A&A,293,521Perrin,Gavel,M.D.,D.T.,Graham,Pennington,J.R.,D.M.,Kalas,&P.,Gates,Lloyd,E.L.J.P.,2004a,Max,Science,C.E.,303,1345Perrin,Gavel,M.D.,D.T.,Graham,Pennington,J.R.,D.M.,Kalas,&P.,Gates,Lloyd,E.L.J.P.,2004b,Max,SPIE,C.E.,Pety,841J.,Gueth,F.,Guilloteau,S.,&Dutrey,A.2006,A&A,458,Piirola,Pyo,T.,V.,etal.Scaltriti,2003,ApJ,F.,&590,Coyne,340G.V.1991,Nature,359,399Racine,R.1968,AJ,73,233Sandell,Sault,R.J.,G.,Teuben,&Weintraub,P.J.,Wright,D.A.1994,M.C.H.A&A,,ASPC,L177,433Schmid-Burgk,J.,Guesten,R.,Mauersberger,R.,Schulz,A.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