Astronomy
The origin of stars
Stellar and laboratory XUV/EUV line ratios in Fe XVIII and Fe XIX
JENAM-2011, SpS3 Oleg Malkov, Olga Dluzhnevskaya, Sergey Karpov, Elena Kilpio, Aleksey Kniazev, Aleksey Mironov, Sergey Sichevskij Institute of Astronomy,
ASIAA Interferometry Summer School – 2006 Introduction – Radio Astronomy Tatsuhiko Hasegawa (ASIAA) 1. Atmospheric window to the electromagnetic waves.
X-ray observations of Dark Particle Accelerators Hiro Matsumoto (KMI, Nagoya University) 1.
Astronomical Distances or Measuring the Universe (Chapters 5 & 6) by Rastorguev Alexey, professor of the Moscow State University and Sternberg Astronomical.
The Trigonometric Parallax B p B = 1 AU = 1.496*10 13 cm d = (1/p[arcsec]) parsec d 1 pc = 3.26 LY ≈ 3*10 18 cm.
The Milky Way. The Milky Way is the great band of light that is best seen in the summer from a dark site. The name "Milky Way" is derived from its appearance.
STAR BIRTH. Guiding Questions Why do astronomers think that stars evolve? What kind of matter exists in the spaces between the stars? Where do new stars.
The Interstellar Medium Chapter 14. Is There Anything Between the Stars? The answer is yes! And that “stuff” forms some of the most beautiful objects.
SALTLIB Proposal for a Stellar Spectral Library using HRS@SALT H. P. Singh, Department of Physics & Astrophysics University of Delhi, Delhi – 110 007,
![The Trigonometric Parallax B p B = 1 AU = 1.496*10 13 cm d = (1/p[arcsec]) parsec d 1 pc = 3.26 LY ≈ 3*10 18 cm.](https://static.fdocuments.net/doc/330x215/56649d925503460f94a783d5/the-trigonometric-parallax-b-p-b-1-au-149610-13-cm-d-1parcsec.jpg)
