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The species was described in 1992 by Glenn Conroy and colleagues, and was at the time the only non-hominin fossil ape known from Southern Africa. The scientists noted that the surrounding area of the discovered specimen included fauna dated at "about 13 ± 1 Myr". [1]
Myr is also used with Mya or Ma. Together they make a reference system, one to a quantity, the other to a particular point in a year numbering system that is time before the present. Myr is deprecated in geology, but in astronomy Myr is standard. Where "myr" is seen in geology, it is usually "Myr" (a unit of mega-years). In astronomy, it is ...
On June 2, 1974, [8] Nu.1, Nu.5 and Nu.10 notes were introduced by the Royal Government of Bhutan, followed by Nu.2, Nu.20, Nu.50, and Nu.100 in 1978. [8] On August 4, 1982, the Royal Monetary Authority of Bhutan Act was enacted, although the RMA did not begin operations until November 1, 1983, and did not issue its own family of notes until 1986.
A myr is a unit of time, one million years, used in astronomy, geology and biology. Myr or MYR may also refer to: Munichi language (ISO 639 language code: myr) Malaysian ringgit, currency of Malaysia by ISO 4217 currency code; Myrtle Beach International Airport (IATA airport code: MYR; ICAO airport code: KMYR), South Carolina, USA
A working timetable (WTT) - (Fr. horaire de service (HDS) or service annuel (SA); N. America Employee timetable) - The data defining all planned train and rolling-stock movements which will take place on the relevant infrastructure during the period for which it is in force; within the EU, it is established once per calendar year. [1]
1% for each MYR 1 over MYR 5,000 0 – 0.75% MYR 20,001 – 35,000 ... and full details and tax tables are available in PDF documents.
The similarity of this kinematic age with the modern age of the Pleiades determined from the Lithium-depletion boundary method (130 ± 20 Myr), [3] led these investigators to conclude that AB Dor Moving Group and Pleiades likely formed around the same time in the same star-forming complex.
The two stars of the RW Aurigae system are separated by 1.448″, equivalent to 237 AU at the distance of RW Aurigae. The primary is a pre-main sequence star with a mass of 1.4 M ☉, while the secondary has a mass of 0.9 M ☉.