Catalogue by Carlos Armando Campos-Saldivar

Nebulae

ccampo13 — 2024-09-17 17:04:02 UTC

Nebulae are interstellar clouds of gas and dust.

HR Diagram

ccampo13 — 2024-09-17 17:09:29 UTC

HR Diagram is a scatter plot of stars showing the relationship between the stars' luminosities and their effective temperatures.

Giants

ccampo13 — 2024-09-17 17:12:29 UTC

A giant star has a larger radius and luminosity than a main-sequence star of the same surface temperature.

Planetary Nebulae

ccampo13 — 2024-09-17 17:17:46 UTC

A planetary nebula is a cloud of gas and dust that forms when a star dies and sheds its outer layers.

Main sequence star

ccampo13 — 2024-09-17 18:18:22 UTC

A main sequence star is any star that has a hot, dense core which fuses hydrogen into helium to produce energy.

Black Hole

ccampo13 — 2024-09-17 20:26:35 UTC

a region of space having a gravitational field so intense that no matter or radiation can escape.

Super Giants

ccampo13 — 2024-09-17 20:27:19 UTC

Super giants are among the most massive and most luminous stars.

Diffuse Nebulae

ccampo13 — 2024-09-17 20:29:12 UTC

Are the clouds of material formed from the explosions of population three, population two stars, and the left over hydrogen and helium from the Big Bang.

Supernova

ccampo13 — 2024-09-17 20:32:02 UTC

A supernova is a massive explosion that occurs when a star dies

White Dwarf

ccampo13 — 2024-09-17 20:33:26 UTC

A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel and lost its outer layers as a planetary nebula.

Supernova remnants

ccampo13 — 2024-09-17 20:34:28 UTC

A supernova remnant is the structure left behind after a star explodes in a supernova

Nova

ccampo13 — 2024-09-17 20:35:24 UTC

A nova is a star that suddenly increases in brightness, becoming much brighter than it was before.