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Arecibo HI Mapping of a Large Sample of Dwarf Irregular Gala

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导读: Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, f

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1

MappedDwarfs

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 20κ¯(6)80V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

arXiv:astro-ph/9601183v1 30 Jan 1996

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1—Continued

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 2080κ¯(6)V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1—Continued

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 2080κ¯(6)V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1—Continued

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 2080κ¯(6)V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1—Continued

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 2080κ¯(6)V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1—Continued

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 2080κ¯(6)V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

TABLE1—Continued

#

(1)NameName(2)R.A.Dec.(3)BTlogD25

(4)Typesource(5) 2080κ¯(6)V⊙ V50

(7)σσ(8)spaceDopt

(9)DH,eDH,max

(10) SdVrms(11)

7

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

AreciboHIMappingofaLargeSampleofDwarfIrregular

Galaxies

G.LyleHo man

Dept.ofPhysics,LafayetteCollege

arXiv:astro-ph/9601183v1 30 Jan 1996E.E.SalpeterCenterforRadiophysicsandSpaceResearch,CornellUniversityB.FarhatDept.ofPhysics,MassachusettsInstituteofTechnologyT.RoosDept.ofPhysics,CornellUniversityH.WilliamsDept.ofPhysicsandAstronomy,UniversityofDelawareandG.HelouInfraredProcessingandAnalysisCenter,CaltechABSTRACTNeutralhydrogenmappingof70dwarfirregular(Sm,ImandBCD)galaxiesisreported,withposition-velocitycontourmaps(andafewcontourmapsinR.A.andDec.)presentedforthoseresolvedbytheArecibobeam.ThegalaxieswereselectedeitherfromtheVirgoClusterCatalog,fromsimilarlyidenti ed eldgalaxies,orfromadistance-limitedsamplewithintheArecibodeclination

range.Wedonot ndanyisolateddwarfswithalargerHItoopticalradiusratiothanDDO154;the“protogalaxy”HI1225+01(Giovanelli&Haynes1989)continuestobeauniqueobjectamongdwarfsthathavebeenmappedinHI.Foralldwarfswithsigni cantrotationweareabletodeterminethesenseofthespin.Foranumberofbetter-resolveddwarfsweareabletodeterminerotationcurves,inmostcasesextendingwellbeyondthelastmeasuredpointinavailablesynthesisarraymaps.Correlationsamongtheseveralmeasuresofgalaxysizeandmassarestudied;inPaperII(Salpeter&Ho man1996)wecombinethesedatawiththoseforthesetofallavailablemappeddwarfirregulargalaxiesandformappedspiralsspanningasimilarrangeofredshiftstoinvestigatevariationsinTully-Fisherrelationsandinsurfacedensitiesasfunctionsofgalaxysizeandluminosityormass.

Neutral hydrogen mapping of 70 dwarf irregular (Sm, Im and BCD) galaxies is reported, with position-velocity contour maps presented for those resolved by the Arecibo beam. The galaxies were selected either from the Virgo Cluster Catalog, from similarly ide

Subjectheadings:Galaxies:Irregular—Galaxies:Kinematicsand

Dynamics—Galaxies:Structure—RadioLines:Galaxies

1.Introduction

Dwarfirregulargalaxiesareaveryheterogeneouslot,rangingfromImVsystemsofsuchlowsurfacebrightnessthattheycanonlyjustbediscernedondeepphotographicplatestoBCDorHIIgalaxiesthatareevidentlyinthethroesofintensestarformation(Sandage&Binggeli1984).Spiralgalaxiesalsohaveawidespreadinsurfacebrightness(Sandage,Binggeli&Tammann1985;Roberts&Haynes1994;Sprayberryetal.1995;McGaugh,Schombert&Bothun1995),andonequestionofinterestistowhatextentthedwarfirregularsaresimplylower-massanaloguesofthespiralsystemsandtowhatextentthe …… 此处隐藏:21312字,全部文档内容请下载后查看。喜欢就下载吧 ……

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