C @(#)dipole.for 17.1.1.1 (ES0-DMD) 01/25/02 17:10:42 C=========================================================================== C Copyright (C) 1995 European Southern Observatory (ESO) C C This program is free software; you can redistribute it and/or C modify it under the terms of the GNU General Public License as C published by the Free Software Foundation; either version 2 of C the License, or (at your option) any later version. C C This program is distributed in the hope that it will be useful, C but WITHOUT ANY WARRANTY; without even the implied warranty of C MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the C GNU General Public License for more details. C C You should have received a copy of the GNU General Public C License along with this program; if not, write to the Free C Software Foundation, Inc., 675 Massachusetss Ave, Cambridge, C MA 02139, USA. C C Corresponding concerning ESO-MIDAS should be addressed as follows: C Internet e-mail: midas@eso.org C Postal address: European Southern Observatory C Data Management Division C Karl-Schwarzschild-Strasse 2 C D 85748 Garching bei Muenchen C GERMANY C=========================================================================== C SUBROUTINE DIPOLE(NIND,X,NPAR,PARAM,Y,DERIV) C+++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ C.COPYRIGHT: Copyright (c) 1987 European Southern Observatory, C all rights reserved C C.VERSION: 1.0 ESO-FORTRAN Conversion, AA 18:01 - 21 DEC 1987 C C.LANGUAGE: F77+ESOext C C.AUTHOR: J.D.PONZ C C-------------------------------------------------------------- C*************************************************** C C IMPLICIT NONE C FIT WITH A LINEAR INFALL MODEL C C Fit the observed radial velocities (in any C reference system) with a dipole velocity C field with respect to this reference C C * * * * * * * * * * * * * * * * * * * * * * * * * C C Independent variables: C C X(1): Galactic longitude C X(2): Galactic latitude C C * * * * * * * * * * * * * * * * * * * * * * * * * C C Free parameters: C C PARAM(1): Solar motion (in km/s) C PARAM(2): Galactic longitude of Apex C PARAM(3): Galactic latitude of Apex C C (All angles are in degrees !) C C * * * * * * * * * * * * * * * * * * * * * * * * * C C Author: O.-G. Richter, ESO Garching C INTEGER NIND,NPAR REAL X(NIND),RAD,D1,A1,A2,D2,BC,BS,A DOUBLE PRECISION Y,PARAM(NPAR),DERIV(NPAR) DATA RAD/1.74532925E-2/ C ! Galactic latitude of object D1 = X(2)*RAD ! Galactic latitude of apex D2 = PARAM(3)*RAD A1 = COS(D1) A2 = COS(D2) D1 = SIN(D1) D2 = SIN(D2) A = A1*A2 ! Difference in galactic longitude BS = (PARAM(2)-X(1))*RAD BC = COS(BS) DERIV(1) = -D1*D2 - A*BC ! Predicted radial velocity Y = DERIV(1)*PARAM(1) DERIV(2) = PARAM(1)*A*SIN(BS)*RAD DERIV(3) = PARAM(1)* (D2*A1*BC-A2*D1)*RAD C RETURN END