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The Location of SHAO
How do barred galaxies get two bars?
1.jpg The Milky Way Galaxy, our home, is not just a spiral galaxy, but a barred spiral. About two thirds of spiral galaxies are classified as barred spirals, among which one type is even more special by hosting two bars. These are termed spiral galaxies with two bars (S2B in short. In Chinese, 2B often...
The 2nd International Association of Planetary Sciences (IAPS) Scientific Assembly (IAPS2015)
P1506025.jpg The 2nd International Association of Planetary Sciences (IAPS) Scientific Assembly (IAPS2015) was held at the Kazan Federal University, 1-4 June 2015, Kazan, Russia, which presented the recent results of the research in space geodesy, dynamical astronomy, astrometry and planetary sciences, and
Scientific Progress
Long term apparent inward motion in the jet of a blazar 3C 66A is discovered [2015.05.21]
A “grand banquet” of science communication organized by SHAO--- Seminar entitle... [2015.04.16]
New research progress in spin alignments of spiral galaxies within the large-scal... [2015.03.23]
Discovery of an Ultra-luminous Quasar with Gigantic Black Hole in the Baby Universe [2015.03.04]
Triaxial halos and discs: red versus blue galaxies [2015.06.23]
The new Hong-Kong/AAO/Strasbourg multi-wavelength and spectroscopic PNe database [2015.06.23]
Why didn't Northern Song China produce a Kepler? [2015.06.08]
The fundamental importance of understanding star cluster evolution [2015.06.01]
The Chinese Annual Astronomy/Astrophysics Meeting First Announcement
The EAVN Tiger Team face-to-face meeting (SHAO-HQ, July 29 2014)
The 2014 Spaceborne Earth Observations and Global Change Workshop and Summer School (First Circular)
8th IVS General Meeting, March 2-7, 2014, Shanghai, China
SHAO was formally established in 1962 following the amalgamation of the former Xujiahui (originally spelt Zi-Ka-Wei) and Sheshan observatories, which were founded by the French Mission Catholique in 1872 and 1900 respectively.
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