Astronomers have completed a 5-year campaign to monitor continuously radio flares from two groups of binary star systems. This survey is of special interest because it provides evidence that certain binary star systems have predictable activity cycles like our Sun.

Astronomers using the National Science Foundation’s newly commissioned Green Bank Telescope have detected remarkably faint radio signals from an 820 year-old pulsar, making it the youngest radio-emitting pulsar known.

A NASA Astronaut who carried a flag bearing the logo of the National Radio Astronomy Observatory on last month’s Shuttle flight returned that flag to the observatory on Friday, April 12, at a ceremony in Socorro.

Ethylene glycol, the chemical commonly used as automobile antifreeze, was discovered recently in a massive interstellar cloud of dust and gas near the center of the Milky Way Galaxy. Scientists used the National Science Foundation’s (NSF) 12 Meter Radio Telescope to detect this organic molecule.

Astronomers using the National Science Foundation’s Very Large Array radio telescope have found a pulsar — a spinning, superdense neutron star — that apparently is considerably younger than previously thought.

Combining the best features of the National Science Foundation’s new Green Bank Telescope in West Virginia with those of the NSF’s Very Large Array in New Mexico, astronomers have produced a vastly improved radio image of the Orion Nebula and developed a valuable new technique for studying star formation and other astrophysical processes.