Then, in principle at least, observers living in a typical galaxy (like our Milky Way) may “see” a different universe than those following the smooth Hubble expansion. Such an apparent effect should be local of course, since peculiar velocities are expected to fade away as we move on to...
The refractor is great in the winter when the seeing is just too poor for the C11, or in the summer when a rich Milky Way target is on the agenda, but truthfully, I'd rather be shooting a small galaxy. I just switched the camera over to the C11 a few days ago in hopes of getti...
What is the size of the sun's diameter in kilometers? How long was Apollo 11 in space? How many stars are in the Milky Way Galaxy? How big is the Sombrero Galaxy? What is the speed of light in space? What are the distances of all planets from the Sun in scientific notation and ...
Using the RR Lyrae surveys Gaia DR3 Specific Objects Study, PanSTARRS1 and ASAS-SN-II, we determine the Milky Way's thick disc scale length and scale height as well as the radial scale length of the galaxy's inner halo. We use a Bayesian approach to estimate these values using two ...
Born: Milky Way Galaxy | Based: Vista, CA Christian Hosoi Pro Skateboarder | Ordained Pastor Author | Inspirational Public Speaker Skateboarding Hall of Fame Inductee Born: Los Angeles, CA | Based: Huntington Beach, CA Tony Alva Pro Skateboarder | Musician, Surfer ...
Then, in principle at least, observers living in a typical galaxy (like our Milky Way) may "see" a different universe than those following the smooth Hub- ble expansion. Such an apparent effect should be local of course, since peculiar velocities are expected to fade away as we move on ...
Using the RR Lyrae surveys Gaia DR3 Specific Objects Study, PanSTARRS1 and ASAS-SN-II, we determine the Milky Way's thick disc scale length and scale height as well as the radial scale length of the galaxy's inner halo. We use a Bayesian approach to estimate these values using two ...
Using the RR Lyrae surveys Gaia DR3 Specific Objects Study, PanSTARRS1 and ASAS-SN-II, we determine the Milky Way's thick disc scale length and scale height as well as the radial scale length of the galaxy's inner halo. We use a Bayesian approach to estimate these values using two ...