-
Low M**** (Latin
Missa Privata) is a
Catholic M**** celebrated by a
priest without the ****istance of
sacred ministers (deacon and subdeacon).
Before 1969...
- environment. Accordingly,
astronomers often group stars by
their m****: Very
low m**** stars, with m****es
below 0.5 M☉, are
fully convective and distribute...
-
classification by
m**** (high, intermediate,
low)
refers to the
optically visible donor, not to the
compact X-ray
emitting accretor.
Low-
m**** X-ray binaries...
- none has yet had time to
evolve to this
point and be observed.)
Low-
m**** stars with a
m**** below about 1.8–2.2 M☉ (depending on composition) do
enter the...
- : §1
After the hydrogen-fusing
period of a main-sequence star of
low or
intermediate m**** ends, such a star will
expand to a red
giant and fuse
helium to...
- was very red and enigmatic,
showing none of the
features expected of a
low-
m**** red dwarf. It
became clear that GD 165B
would need to be
classified as...
- be
typical of the
Solar System's
rocky matter, and a
m**** approximately 2.25
times its
current m****.
Early in the
Solar System's history,
Mercury may have...
- outflows.[jargon]
Observations indicate that the
coldest clouds tend to form
low-
m**** stars,
which are
first observed via the
infrared light they emit inside...
- surprising,
because current theories of
planetary formation suggest that
low-
m**** planets should have
their orbital eccentricity circularized by gravitational...
- a
low-
m**** hypervelocity star
about 408 light-years
distant in the
constellation Canes Venatici. It has an L
spectral type and is
either a
low-
m**** red...
