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OCH.TXT
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1992-07-17
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$regions.mvi
d010
hOur Cosmohood: the 2,367 galaxies within 40 Mpc
mC1,C4,C6,C7,C2,C5,C3
hThe 7 major regions are color-coded
g010,020
$
$u.mvi
;=====local
dl10
mI10,N147,M31,I1613,M33,N6822,MILKYWAY
hOur voyage begins with the Local Group
al10
p
t000,024,015,Each dot or small circle plotted
t000,032,015,on the screen represents one
t000,040,015,galaxy.
p
t000,056,015,Messier galaxies are drawn with
t000,064,015,circles, and non-Messier
t000,072,015,objects appear as dots.
p
t000,088,015,The object colors mean:
t004,096,009, blue = spiral galaxy
t004,104,012, red = elliptical galaxy
t004,112,010,green = irregular galaxy
t004,120,015,white = other galaxy type
p
t380,024,015,The coordinate axes are colored:
t448,032,004,red (positive x-axis),
t448,040,002,green (positive y-axis),
t416,048,001,and blue (positive z-axis).
p
t360,088,015,The length of all 3 coordinate
t360,096,015,axes are the same, and that length
t360,104,015,(in Mpc) is shown in blue at the
t360,112,015,top of the Z axis.
p
t176,264,015,You may press
t288,264,014,PAUSE
t336,264,015,to stop the action,
t204,272,015,and any other key to resume it.
p
t000,306,015,Next, we're going to take a stroll around the Local Group...
p
;=====local group rotated
dl20
mI10,N147,M31,I1613,M33,N6822,MILKYWAY
hA stroll around the Local Group
fl20
fl20
p
t000,024,015,A Group, like the Local Group,
t000,032,015,is the first level of organization
t000,040,015,in the universe above a galaxy.
p
t000,056,015,The members of a group are
t000,064,015,gravitationally bound to each
t000,072,015,other.
p
t400,024,015,The next higher level of
t400,032,015,organization above a group is
t400,040,015,called an association. The
t400,048,015,relation between a group and
t400,056,015,an association is analagous
t400,064,015,to the relation between the
t400,072,015,core and the halo of a galaxy.
p
t400,088,015,Now, we'll zoom out a bit from
t400,096,015,from Local Group, to see the
t400,104,015,Local Association.
p
dl30
mM31,M33,MILKYWAY,N404,N3109
hZooming out to view the Local Association
al30
dl40
mM31,MILKYWAY,N404,N3109
hA stroll around the Local Association
fl40
fl40
p
t000,024,015,So far, we've only been displaying
t000,032,015,the galaxies very near the Milky
t000,040,015,Way. Next, we'll add the galaxies
t000,048,015,which are in the foreground and
t000,056,015,background of this viewpoint, but
t000,064,015,still fairly nearby.
p
;=====comascl
dc10
mM31,M81,M101
hNon Local-Group galaxies are added to the display
ac10
p
t000,024,015,And next, we'll take another step outward
p
dc20
mM31,M81,M101,M94,M64,M82,M83,M63,M51,M106
hWe are zooming outward
fc20
dc30
mM82,M63,M83,M63,M106,M51,M64
hZooming out further...
fc30
dc40
mM82,M106,M83
hZooming out further... and further...
fc40
dc50
m
hZooming out further... and further... and further still.
fc50
dc60
m
hThis is the Coma-Sculptor Cloud, to which the Local Group belongs
ac60
p
t000,024,015,The next higher level of organization
t000,032,015,above an association is called a
t000,040,015,cloud, and the Coma-Sculptor Cloud
t000,048,015,is the cloud in which we reside.
p
mO
hThe Coma-Sculptor Cloud, with a new display on the bottom of the screen.
r
t000,020,015,The three small plots show
t000,030,015,orthographic projections of the
t000,040,015,galaxies on the main display.
p
t000,060,015,The coordinate axes in the small
t000,070,015,plots are colored the same as
t000,080,015,those used in the main plot.
p
t000,100,015,The maximum axis values in the
t000,110,015,small plots is shown in white
t000,120,015,near those plots.
p
t400,020,015,From those orthographic plots,
t400,030,015,you can see that the Coma-
t400,040,015,Sculptor Cloud is a pancake-
t400,050,015,shaped structure which is
t400,060,015,elongated along the X-Y plane.
p
t400,080,015,The next display may help you
t400,090,015,understand the shape of the
t400,100,015,Coma-Sculptor Cloud better.....
p
dc80
m
hThe Coma-Sculptor Cloud
fc80
dc70
ac70
t000,020,015,The X, Y, and Z axes which we have
t000,030,015,been using are the coordinate axes
t000,040,015,of the Cartesian Supergalactic
t000,050,015,Coordinate System.
p
t000,070,015,This coordinate system has its origin
t000,080,015,at the center of the Milky Way.
p
t000,100,015,The X-Y plane lies in the principal
t000,110,015,plane of the Local Supercluster,
t000,120,015,which we'll be viewing a bit later.
p
t000,340,015,Please wait a moment...
hThe Coma-Sculptor Cloud with Equatorial Coordinates superimposed
mN
r
t000,020,015,Equatorial Coordinates for the Northern
t000,030,015,Hemisphere have been superimposed on
t000,040,015,the Coma-Sculptor Cloud.
p
t000,300,015,The positive Supergalactic X axis points
t000,310,015,to the border between Cassiopeia and Perseus.
p
t000,300,015,The positive Supergalactic Z axis points
t000,310,015,to the border between Hercules and Aquila.
p
t000,300,015,The positive Supergalactic Y axis points
t000,310,015,to a spot in Coma Berenices, close to the
t000,320,015,center of the Coma Star Cluster, and not
t000,330,015,far from the North Pole of the Milky Way.
p
t400,300,015,The Coma-Sculptor cloud is
t400,310,015,so named because it stretches
t400,320,015,from Coma (which we now see)
t400,330,015,to Sculptor.
p
t000,340,015,Please wait a moment...
mS
r
t000,020,015,Equatorial Coordinates for the Southern
t000,030,015,Hemisphere have been superimposed on
t000,040,015,the Coma-Sculptor Cloud.
p
t408,010,015,This hemisphere is BEHIND the
t424,020,015,coordinate axes. The spots
t456,030,015,where the negative axes
t448,040,015,intersect the hemisphere
t464,050,015,are marked X,Y, and Z.
p
t000,300,015,The negative Supergalactic X axis points
t000,310,015,very close to Alpha Centauri.
p
t000,300,015,The negative Supergalactic Z axis points
t000,310,015,very close to Sirius.
p
t000,300,015,The negative Supergalactic Y axis points
t000,310,015,to the border between Cetus and Sculptor.
p
t392,300,015,Hence, the Sculptor part of
t392,310,015,the name "Coma-Sculptor Cloud".
p
mG
r
t000,020,015,Now the Galactic Equator (the plane
t000,030,015,of the disk of the Milky Way) has
t000,040,015,been superimposed on the display.
p
t000,060,015,Galactic Lattitude Zero, which points
t000,070,015,to the center of the Milky Way in
t000,080,015,Sagitarrius, is marked with the line.
p
t000,100,015,The Galactic Equator is pretty
t000,110,015,closely aligned with the
t000,120,015,Supergalactic X-Z plane.
p
dc90
hThe Coma-Sculptor Cloud with the Galactic Equator superimposed
fc90
dca0
fca0
p
dc70
mC14+01,C14-01,C14+04,C14+05,C14+06,C14+07,C14+09,C14+10,C14+11,C14+12,C14+13,C14+15
hSeveral associations exist within the Coma-Sculptor Cloud...
ac70
t000,020,015,The color scheme on this display and the
t000,030,015,next few is different. Gray is used for
t000,040,015,for galaxies NOT in one of the displayed
t000,050,015,associations, and other colors are used
t000,060,015,to denote associations.
p
hThe Coma-Sculptor Cloud Associations
mC14+01,C14-01,C14+04,C14+05,C14+06,C14+07,C14+09,C14+10,C14+11,C14+12,C14+13,C14+15
fc80
fc80
p
dc70
m
hNow we're back to the normal color display
ac70
p
;=====spurleo
ds00
m
hThe cloud nearest to the Coma-Sculptor Cloud (the Leo Spur) has been added.
as00
p
ds10
hAnd we're zooming outward a bit for a better look at the Leo Spur.
fs10
ds20
mO
as20
t000,024,015,A Spur is like a Cloud, but is
t000,032,015,is sparsely populated and is
t000,040,015,closely linked with a cloud.
p
t000,056,015,When a filamentary structure
t000,064,015,bifurcates, the less prominent
t000,072,015,feature is often named a Spur.
p
t000,088,015,The relation in space between the
t000,096,015,Coma-Sculptor Cloud and the Leo
t000,104,015,Spur should be easy to see with
t000,112,015,the next frame.
p
ds30
mC14,C15,C15-01
hThe Leo Spur, including the M96 Cluster
fs30
p
;=====zoom
dz10
hWe've now added more distant galaxies to the display, in gray.
fz10
p
dz10
m
hWe've switched all galaxies to normal colors.
fz10
dz20
m
hNow we're zooming out further... the Virgo Cluster is entering from the right
fz20
;=====0cloud
d010
m
hOn the screen now are the 2,367 galaxies within 40 Mpc.
g010,020
p
d010
m
hOur Cosmohood: the 2,367 galaxies within 40 Mpc
g010,020
t000,016,015,In the upcoming animations, we'll
t000,024,015,sweep along one of the coordinate
t000,032,015,axes in 36 divisions of 2.5 Mpc
t000,040,015,each.
p
t000,056,015,The first frame will highlight the
t000,064,015,galaxies in the negative-most 2.5
t000,072,015,Mpc of the axis, the next frame
t000,080,015,will highlight the next
t000,088,015,more-positive 2.5 Mpc, etc.
p
t000,104,015,First, we'll sweep the Z (blue) axis.
p
cz
t000,016,015,Now, we have some structure evident
t000,024,015,on the large-scale. The number of
t000,032,015,galaxies in the 2 or 3 steps near
t000,040,015,Z=0 was as high as all the other
t000,048,015,steps combined.
p
t000,064,015,Here's a rerun of the Z-axis sweep.
p
cz
t000,016,015,What flashed out at us near Z=0
t000,024,015,is the Principal Plane of the
t000,032,015,Local Supercluster.
p
t000,048,015,The Local Supercluster is a
t000,056,015,flattened structure with a dense
t000,064,015,disk component and a sparser halo
t000,072,015,component.
p
t000,088,015,As we mentioned before, the X-Y
t000,096,015,plane of the coordinate axes was
t000,104,015,chosen to lie in the densest part
t000,112,015,of the disk of the Local Supercluster.
p
t000,128,015,Next we'll sweep the Y (green) axis.
p
cy
t000,016,015,The various Y-axis values had an
t000,024,015,approximately even distribution
t000,032,015,of galaxies, certainly much more
t000,040,015,even than the Z-axis sweep.
p
t000,056,015,There were only a few galaxies at the
t000,064,015,negative-most and positive-most values
t000,072,015,(as should be expected -- those are
t000,080,015,the furthest away regions).
p
t000,096,015,There was also a pinching near Y=0,
t000,104,015,which is caused by intervention of
t000,112,015,the disk of the Milky Way galaxy --
t000,120,015,only the nearest galaxies are
t000,128,015,bright enough to show through.
p
t000,144,015,But other than those two explainable
t000,152,015,facts, the distribution is pretty even.
p
t000,168,015,Here's a rerun of the Y-axis sweep.
p
cy
t000,016,015,Finally, we'll sweep the X (red) axis.
p
cx
t000,016,015,Except for an increase in the number
t000,024,015,of galaxies near X=0, this distribution
t000,032,015,was also pretty even. The increase
t000,040,015,near X=0 was not nearly as drastic
t000,048,015,as the one we saw at Z=0.
p
t000,064,015,Here's a rerun of the X-axis sweep.
p
cx
cregions
g040,020
r
t000,016,015,We're now looking edge-on into
t000,024,015,the Milky Way, and can plainly
t000,032,015,see the Zone of Obscuration.
p
t000,048,015,Also, from this viewpoint,
t000,056,015,the 7 major regions are
t000,064,015,well seperated.
p
f030
p
;=====clouds 1x
cregions
t000,016,015,Now we'll cycle through the
t000,024,015,Clouds and Spurs involved in
t000,032,015,Our Cosmohood.
p
t000,016,015,We'll start with the structure
t000,024,015,located in the Principal Plane,
t000,032,015,which was shown in BLUE in this
t000,040,015,view.
p
hThe Principal Plane of the Local Supercluster
mC11,C11-01,C12,C13,C14,C15,C16,C17,C18,C19
g010,020
p
d110
g110,020
p
mC11+04,C11+10,C11+14,C11+24,C11-24
r
p
mC12-01,C12+03,C12+05,C12+06
hThe major cluster in the Ursa Major Cloud
r
p
mC17+01,C17+04
hThe major associations in the Triangulum Spur
r
p
mC19+01
hThe major association in the Pavo-Ara Cloud
r
p
mC11,C11-01,C12,C13,C14,C15,C16,C17,C18,C19
hThe Principal Plane of the Local Supercluster
g120,050
p
;=====clouds 4x and 6x
cregions
t000,016,015,Next we'll look at the structures
t000,024,015,slightly above the Principal Plane,
t000,032,015,which were shown in green and red
t000,040,015,in this view.
p
hStructures slightly above the Principal Plane
mC41,C42,C43,C44,C45,C61,C62,C63,C64,C65,C66
g010,020
p
d410
g410,020
p
mC41+01,C41-01,C41+02,C41+07
hThe major association in the Virgo-Libra Cloud
r
p
mC42+01,C42-01
hThe major association in the CVn-Cam Cloud
r
p
mC43+01
hThe major associations in the CVn spur
r
p
mC44+01
hThe major associations in the Dra Cloud
r
p
mC61+01,C61-01,C61+04,C61-04,C61+11,C61+16
hThe major associations in the Telescopium-Grus Cloud
r
p
mC65+01
hThe major association in the Pegasus Spur
r
p
mC41,C42,C43,C44,C45,C61,C62,C63,C64,C65,C66
hStructures slightly above the Principal Plane
g420,050
p
;=====clouds 7x
cregions
t000,016,015,Next we'll look at the structure
t000,024,015,far above the Principal Plane,
t000,032,015,which was shown in purple
t000,040,015,in this view.
p
hStructures far above the Principal Plane
mC71,C72,C73
g010,020
p
d710
g710,020
g720,050
p
;=====clouds 2x and 5x
cregions
t000,016,015,Next we'll look at the structures
t000,024,015,slightly below the Principal Plane,
t000,032,015,which were shown in brown and yellow
t000,040,015,in this view.
p
hStructures slightly below the Principal Plane
mC21,C22,C23,C24,C51,C52,C53,C54,C55
g010,020
p
d210
t000,016,015,The 5 Clouds listed starting
t000,024,015,with the Fornax-Eridanus Cloud
t000,032,015,are together called the
t000,040,015,Southern Supercluster
p
g210,020
p
mC21+01,C21+03,C21+06,C21+10,C21+12
hThe major associations in the Leo Cloud
r
p
mC22+01
hThe major associations in the Crater Cloud
r
p
mC23+01
hThe major associations in the Centaurus Cloud
r
p
mC51+01,C51-01,C51+04,C51-04,C51+05,C51+07
hThe major associations in the Fornax-Eridanus Cloud
r
p
mC52+01,C52+02,C52+03,C52+06,C52+07
hThe major associations in the Cetus-Aries Cloud
r
p
mC53+01,C53-01,C53+03,C53+07,C53+10
hThe major associations in the Dorado Cloud
r
p
mC54+01,C54+03
hThe major associations in the Antlia Cloud
r
p
mC21,C22,C23,C24,C51,C52,C53,C54,C55
hStructures slightly below the Principal Plane
g220,050
p
;=====clouds 3x
cregions
t000,016,015,Next we'll look at the structures
t000,024,015,far below the Principal Plane,
t000,032,015,which was shown in white
t000,040,015,in this view.
p
hStructures far below the Principal Plane
mC31,C32,C33,C34
g010,020
p
d310
g310,020
p
mC31+02,C31-02
hThe major cluster in the Antlia-Hydra Cloud
r
p
mC31,C32,C33,C34
hStructures far below the Principal Plane
g320,050
p
;=====closing
cregions
t264,264,015,Demo is finished.
t240,274,015,Press Space to restart,
t216,284,015,or ESC to return to Main Menu.
p
p
$
$x.mvi
hSweeping slices of galaxies from negative X to positive X
m
sX-45#-42.5
r
y-43.75,-4,0,-43.75,4,0,004,
sX-42.5#-40
r
y-41.25,-4,0,-41.25,4,0,004,
sX-40#-37.5
r
y-38.75,-4,0,-38.75,4,0,004,
sX-37.5#-35
r
y-36.25,-4,0,-36.25,4,0,004,
sX-35#-32.5
r
y-33.75,-4,0,-33.75,4,0,004,
sX-32.5#-30
r
y-31.25,-4,0,-31.25,4,0,004,
sX-30#-27.5
r
y-28.75,-4,0,-28.75,4,0,004,
sX-27.5#-25
r
y-26.25,-4,0,-26.25,4,0,004,
sX-25#-22.5
r
y-23.75,-4,0,-23.75,4,0,004,
sX-22.5#-20
r
y-21.25,-4,0,-21.25,4,0,004,
sX-20#-17.5
r
y-18.75,-4,0,-18.75,4,0,004,
sX-17.5#-15
r
y-16.25,-4,0,-16.25,4,0,004,
sX-15#-12.5
r
y-13.75,-4,0,-13.75,4,0,004,
sX-12.5#-10
r
y-11.25,-4,0,-11.25,4,0,004,
sX-10#-7.5
r
y-08.75,-4,0,-08.75,4,0,004,
sX-7.5#-5
r
y-06.25,-4,0,-06.25,4,0,004,
sX-5#2.5
r
y-03.75,-4,0,-03.75,4,0,004,
sX-2.5#0
r
y-01.25,-4,0,-01.25,4,0,004,
sX0#2.5
r
y+01.25,-4,0,+01.25,4,0,004,
sX2.5#5
r
y+03.75,-4,0,+03.75,4,0,004,
sX5#7.5
r
y+06.25,-4,0,+06.25,4,0,004,
sX7.5#10
r
y+08.75,-4,0,+08.75,4,0,004,
sX10#12.5
r
y+11.25,-4,0,+11.25,4,0,004,
sX12.5#15
r
y+13.75,-4,0,+13.75,4,0,004,
sX15#17.5
r
y+16.25,-4,0,+16.25,4,0,004,
sX17.5#20
r
y+18.75,-4,0,+18.75,4,0,004,
sX20#22.5
r
y+21.25,-4,0,+21.25,4,0,004,
sX22.5#25
r
y+23.75,-4,0,+23.75,4,0,004,
sX25#27.5
r
y+26.25,-4,0,+26.25,4,0,004,
sX27.5#30
r
y+28.75,-4,0,+28.75,4,0,004,
sX30#32.5
r
y+31.25,-4,0,+31.25,4,0,004,
sX32.5#35
r
y+33.75,-4,0,+33.75,4,0,004,
sX35#37.5
r
y+36.25,-4,0,+36.25,4,0,004,
sX37.5#40
r
y+38.75,-4,0,+38.75,4,0,004,
sX40#42.5
r
y+41.25,-4,0,+41.25,4,0,004,
sX42.5#45
r
y+43.75,-4,0,+43.75,4,0,004,
s
p
$
$y.mvi
hSweeping slices of galaxies from negative Y to positive Y
m
sY-45#-42.5
r
y-4,-43.75,0,4,-43.75,0,002,
sY-42.5#-40
r
y-4,-41.25,0,4,-41.25,0,002,
sY-40#-37.5
r
y-4,-38.75,0,4,-38.75,0,002,
sY-37.5#-35
r
y-4,-36.25,0,4,-36.25,0,002,
sY-35#-32.5
r
y-4,-33.75,0,4,-33.75,0,002,
sY-32.5#-30
r
y-4,-31.25,0,4,-31.25,0,002,
sY-30#-27.5
r
y-4,-28.75,0,4,-28.75,0,002,
sY-27.5#-25
r
y-4,-26.25,0,4,-26.25,0,002,
sY-25#-22.5
r
y-4,-23.75,0,4,-23.75,0,002,
sY-22.5#-20
r
y-4,-21.25,0,4,-21.25,0,002,
sY-20#-17.5
r
y-4,-18.75,0,4,-18.75,0,002,
sY-17.5#-15
r
y-4,-16.25,0,4,-16.25,0,002,
sY-15#-12.5
r
y-4,-13.75,0,4,-13.75,0,002,
sY-12.5#-10
r
y-4,-11.25,0,4,-11.25,0,002,
sY-10#-7.5
r
y-4,-08.75,0,4,-08.75,0,002,
sY-7.5#-5
r
y-4,-06.25,0,4,-06.25,0,002,
sY-5#2.5
r
y-4,-03.75,0,4,-03.75,0,002,
sY-2.5#0
r
y-4,-01.25,0,4,-01.25,0,002,
sY0#2.5
r
y-4,+01.25,0,4,+01.25,0,002,
sY2.5#5
r
y-4,+03.75,0,4,+03.75,0,002,
sY5#7.5
r
y-4,+06.25,0,4,+06.25,0,002,
sY7.5#10
r
y-4,+08.75,0,4,+08.75,0,002,
sY10#12.5
r
y-4,+11.25,0,4,+11.25,0,002,
sY12.5#15
r
y-4,+13.75,0,4,+13.75,0,002,
sY15#17.5
r
y-4,+16.25,0,4,+16.25,0,002,
sY17.5#20
r
y-4,+18.75,0,4,+18.75,0,002,
sY20#22.5
r
y-4,+21.25,0,4,+21.25,0,002,
sY22.5#25
r
y-4,+23.75,0,4,+23.75,0,002,
sY25#27.5
r
y-4,+26.25,0,4,+26.25,0,002,
sY27.5#30
r
y-4,+28.75,0,4,+28.75,0,002,
sY30#32.5
r
y-4,+31.25,0,4,+31.25,0,002,
sY32.5#35
r
y-4,+33.75,0,4,+33.75,0,002,
sY35#37.5
r
y-4,+36.25,0,4,+36.25,0,002,
sY37.5#40
r
y-4,+38.75,0,4,+38.75,0,002,
sY40#42.5
r
y-4,+41.25,0,4,+41.25,0,002,
sY42.5#45
r
y-4,+43.75,0,4,+43.75,0,002,
s
p
$
$z.mvi
hSweeping slices of galaxies from negative Z to positive Z
m
sZ-45#-42.5
r
y-4,0,-43.75,4,0,-43.75,001,
sZ-42.5#-40
r
y-4,0,-41.25,4,0,-41.25,001,
sZ-40#-37.5
r
y-4,0,-38.75,4,0,-38.75,001,
sZ-37.5#-35
r
y-4,0,-36.25,4,0,-36.25,001,
sZ-35#-32.5
r
y-4,0,-33.75,4,0,-33.75,001,
sZ-32.5#-30
r
y-4,0,-31.25,4,0,-31.25,001,
sZ-30#-27.5
r
y-4,0,-28.75,4,0,-28.75,001,
sZ-27.5#-25
r
y-4,0,-26.25,4,0,-26.25,001,
sZ-25#-22.5
r
y-4,0,-23.75,4,0,-23.75,001,
sZ-22.5#-20
r
y-4,0,-21.25,4,0,-21.25,001,
sZ-20#-17.5
r
y-4,0,-18.75,4,0,-18.75,001,
sZ-17.5#-15
r
y-4,0,-16.25,4,0,-16.25,001,
sZ-15#-12.5
r
y-4,0,-13.75,4,0,-13.75,001,
sZ-12.5#-10
r
y-4,0,-11.25,4,0,-11.25,001,
sZ-10#-7.5
r
y-4,0,-08.75,4,0,-08.75,001,
sZ-7.5#-5
r
y-4,0,-06.25,4,0,-06.25,001,
sZ-5#2.5
r
y-4,0,-03.75,4,0,-03.75,001,
sZ-2.5#0
r
y-4,0,-01.25,4,0,-01.25,001,
sZ0#2.5
r
y-4,0,+01.25,4,0,+01.25,001,
sZ2.5#5
r
y-4,0,+03.75,4,0,+03.75,001,
sZ5#7.5
r
y-4,0,+06.25,4,0,+06.25,001,
sZ7.5#10
r
y-4,0,+08.75,4,0,+08.75,001,
sZ10#12.5
r
y-4,0,+11.25,4,0,+11.25,001,
sZ12.5#15
r
y-4,0,+13.75,4,0,+13.75,001,
sZ15#17.5
r
y-4,0,+16.25,4,0,+16.25,001,
sZ17.5#20
r
y-4,0,+18.75,4,0,+18.75,001,
sZ20#22.5
r
y-4,0,+21.25,4,0,+21.25,001,
sZ22.5#25
r
y-4,0,+23.75,4,0,+23.75,001,
sZ25#27.5
r
y-4,0,+26.25,4,0,+26.25,001,
sZ27.5#30
r
y-4,0,+28.75,4,0,+28.75,001,
sZ30#32.5
r
y-4,0,+31.25,4,0,+31.25,001,
sZ32.5#35
r
y-4,0,+33.75,4,0,+33.75,001,
sZ35#37.5
r
y-4,0,+36.25,4,0,+36.25,001,
sZ37.5#40
r
y-4,0,+38.75,4,0,+38.75,001,
sZ40#42.5
r
y-4,0,+41.25,4,0,+41.25,001,
sZ42.5#45
r
y-4,0,+43.75,4,0,+43.75,001,
s
p
$
$010.dcr
40
40
40
0
0
0
13.5
13.5
44
1
40
40
40
0
0
0
3
$
$020.dcr
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
6
$
$030.dcr
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
8
$
$040.dcr
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
7
$
$050.dcr
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
10
$
$110.dcr
1
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
9
$
$120.dcr
1
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
10
$
$210.dcr
2,5
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
9
$
$220.dcr
2,5
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
10
$
$310.dcr
3
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
9
$
$320.dcr
3
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
10
$
$410.dcr
4,6
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
9
$
$420.dcr
4,6
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
10
$
$710.dcr
7
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
9
$
$720.dcr
7
40
40
40
0
0
0
13.5
13.5
44
56
0
48.99
48.99
0
0
0
10
$
$c10.dcr
14
3
3
3
0
0
0
2.5
2.5
2
1
3
3
3
0
0
0
3
$
$c20.dcr
14
3
3
3
0
0
0
2.5
3.3750
2
20
6
6
6
0
0
0
3
$
$c30.dcr
14
6
6
6
0
0
0
3.375
4.25
5
20
9
9
9
0
0
0
3
$
$c40.dcr
14
9
9
9
0
0
0
4.25
5.125
8
20
12
12
12
0
0
0
3
$
$c50.dcr
14
12
12
12
0
0
0
5.1250
6
11
20
15
15
15
0
0
0
3
$
$c60.dcr
14
15
15
15
0
0
0
6
6
12
1
15
15
15
0
0
0
3
$
$c70.dcr
14
15
15
15
0
0
0
6
6
12
1
15
15
15
0
0
0
3
$
$c80.dcr
14
15
15
15
0
0
0
6
6
12
105
0
18.37
18.37
0
0
0
6
$
$c90.dcr
14
15
15
15
0
0
0
6
6
12
15
2.70E+01
0
0
0
0
0
3
$
$ca0.dcr
14
27
0
0
0
0
0
6
6
12
15
15
15
15
0
0
0
3
$
$l10.dcr
14-12
1
1
0.99999999999
0
0
0
1
1
0.8
1
0
0
0
0
0
0
1
$
$l20.dcr
14-12
1
1
1
0
0
0
1
1
0.7
180
0
0
0
0
0
0
2
$
$l30.dcr
14-12,14+12
1
1
1
0
0
0
1
2.5
0.8
60
3
3
3
0
0
0
3
$
$l40.dcr
14-12,14+12
3
3
3
0
0
0
2.5
2.5
2
90
0
0
0
0
0
0
2
$
$s00.dcr
14,15
15
15
15
0
0
0
6
6
14
1
15
15
15
0
0
0
3
$
$s10.dcr
14,15
15
15
15
0
0
0
6
7
14
20
15
15
15
0
0
0
3
$
$s20.dcr
14,15
15
15
15
0
0
0
7
7
14
1
15
15
15
0
0
0
3
$
$s30.dcr
14,15
15
15
15
0
0
0
7
7
14
105
15
15
15
0
0
0
6
$
$z10.dcr
15
15
15
0
0
0
7
7
14
1
15
15
15
0
0
0
3
$
$z20.dcr
15
15
15
0
0
0
7
13.5
14
25
40
40
40
0
0
0
3
$