Radio astronomer Robert Lamme Brown died suddenly of a heart attack on 20 December 2014 in Florence, South Carolina, while traveling to Disney World to visit his grandchildren, to whom he was devoted.Robert Lamme BrownNRAO/AUI/NSFPPT|High resolutionBorn on 17 August 1943 in Los Angeles, Brown was raised in Inglewood, California. While attending the University of California, Berkeley, he worked in Kinsey Anderson’s cosmic-ray research group. He received his BA in 1965. He then went to the University of California, San Diego, where he worked under Robert Gould and was awarded a PhD in 1969. His thesis, “Interstellar absorption of cosmic x rays,” was published in Physical Review D in 1970 and was one of the 100 most cited papers in astronomy and physics during the 1970s.Brown joined the National Radio Astronomy Observatory (NRAO) as a postdoctoral fellow. Although trained as a theorist, he quickly became a skilled observer. A deft manager, he served as the site director of the NRAO’s Green Bank and Tucson facilities, head of its Millimeter Array (MMA) project, and NRAO deputy director.One of Brown’s most significant discoveries, made with Bruce Balick, was the compact radio source at the center of the galaxy, which he later named Sagittarius A*. On 13 and 15 February 1974, the NRAO Green Bank interferometer and a 45-foot antenna in Huntersville, West Virginia, combined to provide enough resolution and sensitivity to detect the faint, compact source. It has since been shown to be coincident with the center of the Milky Way and driven by a massive black hole. The discovery was a fundamental advance in our understanding of galactic nuclei. Brown was also an expert on radio recombination lines, and the 1978 review he wrote with Jay Lockman and Gillian Knapp remains the standard.Brown’s interest in extragalactic astronomy centered on spectral lines in high-redshift objects. He and Morton Roberts were the first to detect neutral hydrogen (HI) in absorption against a quasar, 3C286. Observing HI absorption led Brown to search for carbon monoxide emission from the hyperluminous IR galaxy F10214+4724. He and I found the CO(3→2) rotational line, which extended by a factor of more than 10 the redshift of CO emission detections in IR-rich galaxies. The discovery was a major motivation for the development of the MMA, one of three precursors that merged to become the Atacama Large Millimeter/Submillimeter Array (ALMA).His aptitude for doing several things simultaneously served Brown admirably at the NRAO. He could write effortlessly, and as deputy director he was responsible for drafting the many program plans, long-range plans, and reports required by NSF. A patient person, Brown was well suited to help during negotiations, such as of the agreements with the Soviet Union and Japan for space-based very long baseline interferometry; the merger of the MMA, the Large Millimeter/Submillimeter Array of Japan, and the European Large Southern Array into ALMA; and the frequently contentious process to determine the NRAO’s yearly investment in new instrumentation. His perseverance was essential during the years it took to secure funding to keep the MMA project alive and to join forces with Europe and Japan to form ALMA.A lover of adventure and travel, Brown was the first NRAO member to visit the Atacama Desert of northern Chile as a possible location for the MMA. He immediately recognized its potential and initiated site testing. The location eventually became the site for ALMA, and it has been critical to the array’s stunning success. Indeed, ALMA’s success owes as much to Brown’s efforts as to anyone’s.Brown was enthusiastic about working with young people. He supervised NRAO summer students, mentored postdoctoral fellows, and supervised five graduate students at the University of Virginia.In 2003 Brown left the NRAO to become the director of the National Astronomy and Ionosphere Center (NAIC) and its principal facility, the Arecibo Observatory. Commuting between Cornell University, which was NSF’s contractor for the NAIC, and Arecibo in Puerto Rico, Brown made many improvements to the observatory’s operation.To channel his energy after he retired in 2008, Brown and his wife, Karen, opened an ice cream parlor in Corolla, on the Outer Banks of North Carolina. He defined his shop role as “chief financial officer and head of janitorial services.”Friendly, outgoing, and well liked, Brown had an infectious laugh that resonated in the halls of the NRAO. He is missed by his family, friends, and colleagues.© 2015 American Institute of Physics.
Read full abstract
Sep 1, 2016
A.-K Baczko + 15
Open Access
