supernova remnant

  • Exploring the Milky Way’s Nucleus

    Exploring the Milky Way’s Nucleus

    Here is an edge-on illustration of our Milky Way Galaxy. (Keep in mind that the disk actually stretches quite a bit farther out from the budge than is apparent in this illustration. Proportionally, its full diameter makes its thickness less…

    Continue reading →

  • Unique Neutron Stars

    Unique Neutron Stars

    Neutron stars — the compact remains of massive stars that have gone supernova — are some of the most extreme objects in the universe, narrowly beaten by black holes (and, as we’ll talk about in future posts, active galaxies and…

    Continue reading →

  • Pulsars as Neutron Stars

    Pulsars as Neutron Stars

    For those of you who missed my last couple of posts, allow me to introduce the neutron star: a stellar remnant similar to a white dwarf, but much denser, so dense that its protons and electrons have combined to form…

    Continue reading →

  • What is a Pulsar?

    What is a Pulsar?

    Imagine you’re observing the sky with a radio telescope. Observing the faintest, lowest-energy photons the universe has to offer is your specialty. You study interstellar dust clouds, protostars, and lots more. One day, though, something interesting pops up in your…

    Continue reading →

  • Why Neutron Stars Should Exist

    Why Neutron Stars Should Exist

    Above is a theoretical rendering of a white dwarf, the collapsed husk of a low-mass or medium-mass star. Interestingly enough, these strange cosmic objects — which begin their existence as intensely hot balls of carbon the size of the Earth…

    Continue reading →

  • What Exactly are Supernovae?

    What Exactly are Supernovae?

    This is one topic I bet you guys have been looking forward to since I first started posting about stellar evolution. Well, I won’t disappoint you! In my last post, we covered how a massive star gets to the point…

    Continue reading →