Citation: Gl. Verschuur, NEW ZEEMAN-EFFECT MEASUREMENTS OF THERMAL OH SOURCES S106, ORION-B, B1, AND L134 AT 1665 AND 1667 MHZ, The Astronomical journal, 112(6), 1996, pp. 2718-2725
Citation: Gl. Verschuur, INTERSTELLAR NEUTRAL HYDROGEN FILAMENTS AT HIGH GALACTIC LATITUDES AND THE BENNETT PINCH, Astrophysics and space science, 227(1-2), 1995, pp. 187-198
Citation: Gl. Verschuur, ZEEMAN-EFFECT OBSERVATIONS OF H-I EMISSION PROFILES .1. MAGNETIC-FIELD LIMITS FOR 3 REGIONS BASED ON OBSERVATIONS CORRECTED FOR POLARIZED BEAM STRUCTURE, The Astrophysical journal, 451(2), 1995, pp. 624-644
Citation: Gl. Verschuur, ZEEMAN-EFFECT OBSERVATIONS OF H-I EMISSION PROFILES .2. RESULTS OF ANATTEMPT TO CONFIRM PREVIOUS CLAIMS OF FIELD DETECTIONS, The Astrophysical journal, 451(2), 1995, pp. 645-659
Citation: Gl. Verschuur et L. Magnani, ON THE NATURE OF 21 CM EMISSION PROFILE STRUCTURE AT HIGH GALACTIC LATITUDE - IMPLICATIONS FOR THE WARM NEUTRAL MEDIUM, The Astronomical journal, 107(1), 1994, pp. 287-297
Citation: Gl. Verschuur, A SUPERSHELL MODEL FOR THE HIGH-VELOCITY AND INTERMEDIATE-VELOCITY NEUTRAL HYDROGEN CLOUDS, The Astrophysical journal, 409(1), 1993, pp. 205-233
Citation: Gl. Verschuur, BEAM BIAS - THE INFLUENCE OF BEAMWIDTH ON OBSERVATIONS OF H-I CLOUDS AND THE SIGNIFICANCE OF DERIVED CLOUD DENSITIES, The Astronomical journal, 106(6), 1993, pp. 2580-2586