LSRD¶
- class astropy.coordinates.LSRD(*args, copy=True, representation_type=None, differential_type=None, **kwargs)[source]¶
Bases:
BaseRADecFrame
A coordinate or frame in the Dynamical Local Standard of Rest (LSRD)
This frame is defined as a velocity of U=9 km/s, V=12 km/s, and W=7 km/s in Galactic coordinates or 16.552945 km/s towards l=53.13 b=25.02. This is defined in:
Delhaye 1965, Solar Motion and Velocity Distribution of Common Stars.
This coordinate frame is axis-aligned and co-spatial with
ICRS
, but has a velocity offset relative to the solar system barycenter to remove the peculiar motion of the sun relative to the LSRD.Attributes Summary
Default representation for differential data (e.g., velocity)
Default representation for position data
Mapping for frame-specific component names
Attributes Documentation
- default_differential¶
Default representation for differential data (e.g., velocity)
- default_representation¶
Default representation for position data
- frame_attributes = {}¶
- frame_specific_representation_info¶
Mapping for frame-specific component names
- name = 'lsrd'¶