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Diffstat (limited to 'math/slalib/rvgalc.f')
-rw-r--r-- | math/slalib/rvgalc.f | 87 |
1 files changed, 87 insertions, 0 deletions
diff --git a/math/slalib/rvgalc.f b/math/slalib/rvgalc.f new file mode 100644 index 00000000..173c7d92 --- /dev/null +++ b/math/slalib/rvgalc.f @@ -0,0 +1,87 @@ + REAL FUNCTION slRVGA (R2000, D2000) +*+ +* - - - - - - - +* R V G A +* - - - - - - - +* +* Velocity component in a given direction due to the rotation +* of the Galaxy (single precision) +* +* Given: +* R2000,D2000 real J2000.0 mean RA,Dec (radians) +* +* Result: +* Component of dynamical LSR motion in direction R2000,D2000 (km/s) +* +* Sign convention: +* The result is +ve when the dynamical LSR is receding from the +* given point on the sky. +* +* Note: The Local Standard of Rest used here is a point in the +* vicinity of the Sun which is in a circular orbit around +* the Galactic centre. Sometimes called the "dynamical" LSR, +* it is not to be confused with a "kinematical" LSR, which +* is the mean standard of rest of star catalogues or stellar +* populations. +* +* Reference: The orbital speed of 220 km/s used here comes from +* Kerr & Lynden-Bell (1986), MNRAS, 221, p1023. +* +* Called: +* slCS2C, slVDV +* +* P.T.Wallace Starlink 23 March 1994 +* +* Copyright (C) 1995 Rutherford Appleton Laboratory +* +* License: +* This program is free software; you can redistribute it and/or modify +* it under the terms of the GNU General Public License as published by +* the Free Software Foundation; either version 2 of the License, or +* (at your option) any later version. +* +* This program is distributed in the hope that it will be useful, +* but WITHOUT ANY WARRANTY; without even the implied warranty of +* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the +* GNU General Public License for more details. +* +* You should have received a copy of the GNU General Public License +* along with this program (see SLA_CONDITIONS); if not, write to the +* Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor, +* Boston, MA 02110-1301 USA +* +* Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. +*- + + IMPLICIT NONE + + REAL R2000,D2000 + + REAL VA(3), VB(3) + + REAL slVDV + +* +* LSR velocity due to Galactic rotation +* +* Speed = 220 km/s +* Apex = L2,B2 90deg, 0deg +* = RA,Dec 21 12 01.1 +48 19 47 J2000.0 +* +* This is expressed in the form of a J2000.0 x,y,z vector: +* +* VA(1) = X = -SPEED*COS(RA)*COS(DEC) +* VA(2) = Y = -SPEED*SIN(RA)*COS(DEC) +* VA(3) = Z = -SPEED*SIN(DEC) + + DATA VA / -108.70408, +97.86251, -164.33610 / + + + +* Convert given J2000 RA,Dec to x,y,z + CALL slCS2C(R2000,D2000,VB) + +* Compute dot product with LSR motion vector + slRVGA=slVDV(VA,VB) + + END |