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The Galactic Centre contains a supermassive black hole with a mass of four million Suns 1 within an environment that differs markedly from that of the Galactic disk. Although the black hole is essentially quiescent in the broader context of active galactic nuclei, X-ray observations have provided evidence for energetic outbursts from its surroundings 2 . Also, although the levels of star formation in the Galactic Centre have been approximately constant over the past few hundred million years, there is evidence of increased short-duration bursts 3 , strongly influenced by the interaction of the black hole with the enhanced gas density present within the ring-like central molecular zone 4 at Galactic longitude | l | < 0.7 degrees and latitude | b | < 0.2 degrees. The inner 200-parsec region is characterized by large amounts of warm molecular gas 5 , a high cosmic-ray ionization rate 6 , unusual gas chemistry, enhanced synchrotron emission 7 , 8 , and a multitude of radio-emitting magnetized filaments 9 , the origin of which has not been established. Here we report radio imaging that reveals a bipolar bubble structure, with an overall span of 1 degree by 3 degrees (140 parsecs × 430 parsecs), extending above and below the Galactic plane and apparently associated with the Galactic Centre. The structure is edge-brightened and bounded, with symmetry implying creation by an energetic event in the Galactic Centre. We estimate the age of the bubbles to be a few million years, with a total energy of 7 × 10 52  ergs. We postulate that the progenitor event was a major contributor to the increased cosmic-ray density in the Galactic Centre, and is in turn the principal source of the relativistic particles required to power the synchrotron emission of the radio filaments within and in the vicinity of the bubble cavities. Radio observations show a bipolar bubble structure of size 140 parsecs by 430 parsecs both above and below the Galactic Centre.

In 1971 he supervised the organisation of the general pathology department in the Glasgow Royal Infirmary before moving in 1974 to the Western Infirmary, Glasgow, where he continued to provide a smooth environment in the pathology department until he retired in 1984.

The Galactic Centre contains a supermassive black hole with a mass of 4 million suns within an environment that differs markedly from that of the Galactic disk. While the black hole is essentially quiescent in the broader context of active galactic nuclei, X-ray observations have provided evidence for energetic outbursts from its surroundings. Also, while the levels of star formation in the Galactic Centre have been approximately constant over the last few hundred Myr, there is evidence of elevated short-duration bursts, strongly influenced by interaction of the black hole with the enhanced gas density present within the ring-like Central Molecular Zone at Galactic longitude |l| < 0.7 degrees and latitude |b| < 0.2 degrees. The inner 200 pc region is characterized by large amounts of warm molecular gas, a high cosmic ray ionization rate, unusual gas chemistry, enhanced synchrotron emission, and a multitude of radio-emitting magnetised filaments, the origin of which has not been established. Here we report radio imaging that reveals bipolar bubbles spanning 1 degree x 3 degrees (140 parsecs x 430 parsecs), extending above and below the Galactic plane and apparently associated with the Galactic Centre. The structure is edge-brightened and bounded, with symmetry implying creation by an energetic event in the Galactic Centre. We estimate the age of the bubbles to be a few million years, with a total energy of 7 x 10^52 ergs. We postulate that the progenitor event was a major contributor to the increased cosmic-ray density in the Galactic Centre, and is in turn the principal source of the relativistic particles required to power the synchrotron emission of the radio filaments within and in the vicinity of the bubble cavities.

We present the SARAO MeerKAT Galactic Plane Survey (SMGPS), a 1.3 GHz continuum survey of almost half of the Galactic Plane (251\\deg \\(\\le l \\le\\) 358\\deg and 2\\deg \\(\\le l \\le\\) 61\\deg at \\(|b| \\le 1.5\\deg \\)). SMGPS is the largest, most sensitive and highest angular resolution 1 GHz survey of the Plane yet carried out, with an angular resolution of 8\" and a broadband RMS sensitivity of \\(\\sim\\)10--20 \\(\\mu\\) Jy/beam. Here we describe the first publicly available data release from SMGPS which comprises data cubes of frequency-resolved images over 908--1656 MHz, power law fits to the images, and broadband zeroth moment integrated intensity images. A thorough assessment of the data quality and guidance for future usage of the data products are given. Finally, we discuss the tremendous potential of SMGPS by showcasing highlights of the Galactic and extragalactic science that it permits. These highlights include the discovery of a new population of non-thermal radio filaments; identification of new candidate supernova remnants, pulsar wind nebulae and planetary nebulae; improved radio/mid-IR classification of rare Luminous Blue Variables and discovery of associated extended radio nebulae; new radio stars identified by Bayesian cross-matching techniques; the realisation that many of the largest radio-quiet WISE HII region candidates are not true HII regions; and a large sample of previously undiscovered background HI galaxies in the Zone of Avoidance.

Ian Alexander McGregor, plastic surgeon; born June 6, 1921, died April 13, 1998 The death of Ian McGregor brings sadness to his many friends and colleagues worldwide. He was a giant in plastic surgery and a staunch friend. His post-graduate training began with a year in the Anatomy Department of the university and a love of anatomical detail remained with him and stood him in good stead. His definitive appointment was as consultant plastic surgeon at Canniesburn Hospital, of which he was director from 1980-86, and he contributed largely to the eminence of Canniesburn Hospital as an international centre of excellence for plastic surgical care and training. He received numerous honours from the US, Canada, Aus- tralia, and Europe. In 1984-86 he was president of the Royal College of Physicians and Surgeons of Glasgow, and in 1979 president of the British Association of Plastic Surgeons. His book, Fundamental Techniques in Plastic Surgery, first published in 1960, is now in its ninth edition: a recent review suggested that a copy should be fixed to the wall of every cas-ualty department in the land. His works include Cancer of the Face and Mouth, written in collaboration with his wife, [Mary Vint], and many chapters in textbooks.

At a regular meeting of Mechanics' Mutual Protection No. 5, of New York, held on the evening of the 21st inst., the following preamble and resolutions were adopted unanimously.