-
Milky Way,
though many
others outside the
galaxy have been seen
since S
Andromedae in 1885. SN 1987A in the
Large Magellanic Cloud was
visible to the naked...
- OS
Andromedae,
known also as
Nova Andromedae 1986, is a
classical nova that
appeared in the
constellation Andromeda during 1986. It was
discovered at...
- IW
Andromedae is a
binary star
system in the
northern constellation of Andromeda,
abbreviated IW And. It is the
prototype of a
class of
variable stars...
- Z
Andromedae is a
binary star
system consisting of a red
giant and a
white dwarf. It is the
prototype of a type of
cataclysmic variable star
known as symbiotic...
- V455
Andromedae (often
abbreviated to V455 And) is a
dwarf nova in the
constellation Andromeda. It has a
typical apparent visual magnitude of 16.5, but...
-
length of 330 days, thus is
classified as a
dwarf nova of the SS
Cygni type. The
system of DX
Andromedae consists of a
white dwarf accreting matter from...
- RX
Andromedae is a
variable star in the
constellation of Andromeda.
Although it is
classified as a
dwarf nova of the Z
Camelopardalis (UGZ) type, it has...
-
lines are
shown in
novae and
dwarf novae outbursts, and PX
Andromedae is
often described as
nova-like
although it does not
shown outbursts with
large increases...
-
supernova (known as S
Andromedae) was seen in Andromeda, the
first and so far only one
observed in that galaxy. At the time, it was
called "
Nova 1885"—the difference...
- Rupen, M. P.; Stone, R. P. S. (2006-01-10). "A "Combination
Nova"
Outburst in Z
Andromedae:
Nuclear S****
Burning Triggered by a Disk Instability". The...
