- GK
****i (also
Nova ****i 1901) was a
bright nova first observed on
Earth in 1901. It was
discovered by
Thomas David Anderson, an
Edinburgh clergyman...
-
progenitor stars via
light echos as
observed with the
spherical s**** of
Nova ****i 1901 or the
energies remaining in the
expanding bubbles like T Pyxidis...
- ****umed the
possibility of
expansion of the
bright ring (nebula)
around Nova ****i 1901 with a
velocity exceeding that of light." He continues: "The comparison...
-
light bubble around Nova ****i (1901).
Thought to be a nebula, the
visual appearance was
actually caused by
light from the
nova event reflected from...
- V392
****i, also
known as
Nova ****i 2018, is a
bright nova in the
constellation ****us
discovered on
April 29, 2018. It was
previously known as a dwarf...
-
notable star
systems in ****us
include X
****i, a
binary system containing a
neutron star, and GK
****i, a
nova that
peaked at
magnitude 0.2 in 1901. The...
- V
****i, also
known as
Nova ****i 1887 was
discovered by
Williamina Fleming on a
Harvard College Observatory objective-prism
photograph taken on 3 November...
- Rodríguez-Gil, P.; Verro, K.; Kolka, I. (2014). "A
Dynamical Study of the
Nova Remnant of GK
****i /
Stella Novae: Past and ****ure Decades.".
Stellar Novae: Past...
- ****us and one of the
first non-
nova variable stars to be discovered.
Algol is a three-star system,
consisting of Beta
****i Aa1, Aa2, and Ab – in which...
-
Aurigae is
classified as a slow
nova,
similar to DQ Herculis. Like DQ Herculis, WZ Sagittae,
Nova ****i 1901 and
Nova Aquilae 1918, it is a very close...
