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We present an HI absorption survey of the central 250 pc of the Galaxy. Very Large Array (VLA) observations were made at 21 cm in the DnC and CnB con gurations and have a resolution of 15"(0.6 pc at ...
A group of four compact HII regions associated with the well-known 50 km/s molecular cloud is the closest site of on-going star formation to the dynamical center of the Galaxy, at a projected distance...
We present results from integral field spectroscopy with the Potsdam Multi-Aperture Spectrograph at the 3.5m telescope at Calar Alto Observatory of the intense star-forming region [HL90] 111 at the ce...
We present significantly improved proper motion measurements of the Milky Way's central stellar cluster. These improvements are made possible by refining our astrometric reference frame with a new geo...
Catching a runaway in the Galactic Center:a study of the IRS8 bowshock。
VLA Detection of a Double Radio Source at the Center of the HH 288 Quadrupolar Outflow。
A new method to find the potential center of N-Body systems。
The Center for Theoretical Astrophysics works on outstanding problems in theoretical astrophysics, general relativity, and cosmology. Members of the Center work out of Loomis Laboratory of Physics, th...
The Harvard-Smithsonian Center for Astrophysics (CfA) is a collaboration between the Harvard College Observatory (HCO) and the Smithsonian Astrophysical Observatory (SAO) . Many CfA staff members are ...
November 30, 2006,Astrobiology is an exciting new scientific program and discipline that has been initially funded and encouraged by NASA. Today, we celebrate the formation of the Carl Sagan Center fo...

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