Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_AS/103/67 into FORTRAN code for loading all data files into arrays.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Apr-18
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/A+AS/103/67 Evolutionary sequences with MC metallicities (de Loore+ 1994)
*================================================================================
*Evolutionary sequences for massive close binary stars with Magellanic Cloud
*metallicities with Rogers-Iglesias opacities
* de Loore C., Vanbeveren D.
* <Astron. Astrophys. Suppl. Ser. 103, 67 (1994)>
* =1994A&AS..103...67D
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'lmc.dat' ! LMC abundances (Table3 to Table15)
integer*4 nr__
parameter (nr__=181) ! Number of records
character*175 ar__ ! Full-size record
integer*4 IM1 (nr__) ! (Sun) Initial mass of the primary
real*4 IM2 (nr__) ! (Sun) Initial mass of the secondary
character*10 Phase (nr__) ! See note (1)
real*4 Age (nr__) ! (yr) Evolutionary stage
real*4 M1 (nr__) ! (solMass) Mass of the primary
real*4 ML1 (nr__) ! (solMass/yr) Mass loss rate of the primary
real*4 logTeff1 (nr__) ! ([K]) Effective temperature of the primary
real*4 logL1 (nr__) ! ([solLum]) Luminosity of the primary
real*4 XC1 (nr__) ! Central hydrogen content of the primary
real*4 YC1 (nr__) ! Central helium content of the primary
real*4 XAT1 (nr__) ! Surface hydrogen abundance of the primary
real*4 Rad1 (nr__) ! (solRad) Radius of the primary
real*4 MCC1 (nr__) ! (Sun) Convective core mass of the primary
real*8 Period (nr__) ! (d) ? Orbital period
real*4 M2 (nr__) ! (solMass) ? Mass of the secondary
real*4 ML2 (nr__) ! (solMass/yr) ? Mass loss rate of the secondary
real*4 logTeff2 (nr__) ! ([K]) ? Effective temperature of the secondary
real*4 logL2 (nr__) ! ([solLum]) ? Luminosity of the secondary
real*4 XC2 (nr__) ! ? Central hydrogen content of the secondary
real*4 YC2 (nr__) ! ? Central helium content of the secondary
real*4 XAT2 (nr__) ! ? Surface hydrogen content of the secondary
real*4 Rad2 (nr__) ! (solRad) ? Radius of the secondary
real*4 MCC2 (nr__) ! (solMass) ? Convective core mass of the secondary
*Note (1): The different phases is as follows:
* ZAMS: Zero Age Main Sequence
* RP1: Red Point of the primary component
* Xc1=0: end of core hydrogen burning of the primary
* RLOFi: onset of a case B of Roche Lobe Overflow
* Lmin: minimum luminosity of the primary
* Xat<0.76 (SMC, or 0.74 (LMC)): hydrogen abundance of the primary drops
* below its initial value
* CHeB1i: onset of core helium burning of the primary
* VHeB1i: onset of core helium burning of the primary
* RLOFf: end of Roche Lobe Overflow
* Yc1=0: end of core helium burning of the primary
* RP2: red point of the secondary
* Xc2=0: end core hydrogen burning of the secondary.
* Teffmin2: minimum of the effective temperature of the secondary
* Teffmax2: maximum of the effective temperature of the secondary
* WNL1,WNE1, WC1 denote the onset of the different Wolf-Rayet phases,
* the WNL,WNE and WC-phases of the primary.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'smc.dat' ! SMC abundances (Table16 to Table29)
integer*4 nr__1
parameter (nr__1=176) ! Number of records
character*175 ar__1 ! Full-size record
integer*4 IM1_1 (nr__1) ! (Sun) Initial mass of the primary
real*4 IM2_1 (nr__1) ! (Sun) Initial mass of the secondary
character*10 Phase_1 (nr__1) ! See note (1)
real*4 Age_1 (nr__1) ! (yr) Evolutionary stage
real*4 M1_1 (nr__1) ! (solMass) Mass of the primary
real*4 ML1_1 (nr__1) ! (solMass/yr) Mass loss rate of the primary
real*4 logTeff1_1 (nr__1) ! ([K]) Effective temperature of the primary
real*4 logL1_1 (nr__1) ! ([solLum]) Luminosity of the primary
real*4 XC1_1 (nr__1) ! Central hydrogen content of the primary
real*4 YC1_1 (nr__1) ! Central helium content of the primary
real*4 XAT1_1 (nr__1) ! Surface hydrogen abundance of the primary
real*4 Rad1_1 (nr__1) ! (solRad) Radius of the primary
real*4 MCC1_1 (nr__1) ! (Sun) Convective core mass of the primary
real*8 Period_1 (nr__1) ! (d) ? Orbital period
real*4 M2_1 (nr__1) ! (solMass) ? Mass of the secondary
real*4 ML2_1 (nr__1) ! (solMass/yr) ? Mass loss rate of the secondary
real*4 logTeff2_1 (nr__1) ! ([K]) ? Effective temperature of the secondary
real*4 logL2_1 (nr__1) ! ([solLum]) ? Luminosity of the secondary
real*4 XC2_1 (nr__1) ! ? Central hydrogen content of the secondary
real*4 YC2_1 (nr__1) ! ? Central helium content of the secondary
real*4 XAT2_1 (nr__1) ! ? Surface hydrogen content of the secondary
real*4 Rad2_1 (nr__1) ! (solRad) ? Radius of the secondary
real*4 MCC2_1 (nr__1) ! (solMass) ? Convective core mass of the secondary
*Note (1): The different phases is as follows:
* ZAMS: Zero Age Main Sequence
* RP1: Red Point of the primary component
* Xc1=0: end of core hydrogen burning of the primary
* RLOFi: onset of a case B of Roche Lobe Overflow
* Lmin: minimum luminosity of the primary
* Xat<0.76 (SMC, or 0.74 (LMC)): hydrogen abundance of the primary drops
* below its initial value
* CHeB1i: onset of core helium burning of the primary
* VHeB1i: onset of core helium burning of the primary
* RLOFf: end of Roche Lobe Overflow
* Yc1=0: end of core helium burning of the primary
* RP2: red point of the secondary
* Xc2=0: end core hydrogen burning of the secondary.
* Teffmin2: minimum of the effective temperature of the secondary
* Teffmax2: maximum of the effective temperature of the secondary
* WNL1,WNE1, WC1 denote the onset of the different Wolf-Rayet phases,
* the WNL,WNE and WC-phases of the primary.
C=============================================================================
C Loading file 'lmc.dat' ! LMC abundances (Table3 to Table15)
C Format for file interpretation
1 format(
+ I2,1X,F4.1,A10,1X,E12.6,1X,F5.2,2X,E11.4,3X,F5.3,3X,F5.3,1X,
+ F5.3,1X,F5.3,1X,F5.3,3X,F5.2,2X,F5.2,1X,F8.4,F6.2,1X,E11.4,3X,
+ F5.3,3X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,3X,F5.2,3X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'lmc.dat')
write(6,*) '....Loading file: lmc.dat'
do i__=1,181
read(1,'(A175)')ar__
read(ar__,1)
+ IM1(i__),IM2(i__),Phase(i__),Age(i__),M1(i__),ML1(i__),
+ logTeff1(i__),logL1(i__),XC1(i__),YC1(i__),XAT1(i__),
+ Rad1(i__),MCC1(i__),Period(i__),M2(i__),ML2(i__),
+ logTeff2(i__),logL2(i__),XC2(i__),YC2(i__),XAT2(i__),
+ Rad2(i__),MCC2(i__)
if(ar__(100:107) .EQ. '') Period(i__) = rNULL__
if(ar__(108:113) .EQ. '') M2(i__) = rNULL__
if(ar__(115:125) .EQ. '') ML2(i__) = rNULL__
if(ar__(129:133) .EQ. '') logTeff2(i__) = rNULL__
if(ar__(137:141) .EQ. '') logL2(i__) = rNULL__
if(ar__(143:147) .EQ. '') XC2(i__) = rNULL__
if(ar__(149:153) .EQ. '') YC2(i__) = rNULL__
if(ar__(155:159) .EQ. '') XAT2(i__) = rNULL__
if(ar__(163:167) .EQ. '') Rad2(i__) = rNULL__
if(ar__(171:175) .EQ. '') MCC2(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ IM1(i__),IM2(i__),Phase(i__),Age(i__),M1(i__),ML1(i__),
+ logTeff1(i__),logL1(i__),XC1(i__),YC1(i__),XAT1(i__),
+ Rad1(i__),MCC1(i__),Period(i__),M2(i__),ML2(i__),
+ logTeff2(i__),logL2(i__),XC2(i__),YC2(i__),XAT2(i__),
+ Rad2(i__),MCC2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'smc.dat' ! SMC abundances (Table16 to Table29)
C Format for file interpretation
2 format(
+ I2,1X,F4.1,A10,1X,E12.6,1X,F5.2,2X,E11.4,3X,F5.3,3X,F5.3,1X,
+ F5.3,1X,F5.3,1X,F5.3,3X,F5.2,2X,F5.2,1X,F8.4,F6.2,1X,E11.4,3X,
+ F5.3,3X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,3X,F5.2,3X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'smc.dat')
write(6,*) '....Loading file: smc.dat'
do i__=1,176
read(1,'(A175)')ar__1
read(ar__1,2)
+ IM1_1(i__),IM2_1(i__),Phase_1(i__),Age_1(i__),M1_1(i__),
+ ML1_1(i__),logTeff1_1(i__),logL1_1(i__),XC1_1(i__),YC1_1(i__),
+ XAT1_1(i__),Rad1_1(i__),MCC1_1(i__),Period_1(i__),M2_1(i__),
+ ML2_1(i__),logTeff2_1(i__),logL2_1(i__),XC2_1(i__),YC2_1(i__),
+ XAT2_1(i__),Rad2_1(i__),MCC2_1(i__)
if(ar__1(100:107) .EQ. '') Period_1(i__) = rNULL__
if(ar__1(108:113) .EQ. '') M2_1(i__) = rNULL__
if(ar__1(115:125) .EQ. '') ML2_1(i__) = rNULL__
if(ar__1(129:133) .EQ. '') logTeff2_1(i__) = rNULL__
if(ar__1(137:141) .EQ. '') logL2_1(i__) = rNULL__
if(ar__1(143:147) .EQ. '') XC2_1(i__) = rNULL__
if(ar__1(149:153) .EQ. '') YC2_1(i__) = rNULL__
if(ar__1(155:159) .EQ. '') XAT2_1(i__) = rNULL__
if(ar__1(163:167) .EQ. '') Rad2_1(i__) = rNULL__
if(ar__1(171:175) .EQ. '') MCC2_1(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ IM1_1(i__),IM2_1(i__),Phase_1(i__),Age_1(i__),M1_1(i__),
+ ML1_1(i__),logTeff1_1(i__),logL1_1(i__),XC1_1(i__),YC1_1(i__),
+ XAT1_1(i__),Rad1_1(i__),MCC1_1(i__),Period_1(i__),M2_1(i__),
+ ML2_1(i__),logTeff2_1(i__),logL2_1(i__),XC2_1(i__),YC2_1(i__),
+ XAT2_1(i__),Rad2_1(i__),MCC2_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end