70/551 Open-ended Working Group on the Fourth Special Sessionof the General Assembly Devoted to Disarmament

2008 ◽  
Vol 4 (T27A) ◽  
pp. 313-315
Author(s):  
Eugene F. Milone ◽  
Andrew T. Young ◽  
Eva Bauwens ◽  
Roger A. Bell ◽  
Michael S. Bessell ◽  
...  

As we have noted before, the WG-IR was created following a Joint Commission Meeting at the IAU General Assembly in Baltimore in 1988, a meeting that provided both diagnosis and prescription for the perceived ailments of infrared photometry at the time. The results were summarized in Milone (1989). The challenges involve how to explain the failure to systematically achieve the milli-magnitude precision expected of infrared photometry and an apparent 3% limit on system transformability. The proposed solution was to re-define the broadband Johnson system, the passbands of which had proven so unsatisfactory that over time effectively different systems proliferated although bearing the same JHKLMNQ designations; the new system needed to be better positioned and centered in the atmospheric windows of the Earth's atmosphere, and the variable water vapour content of the atmosphere needed to be measured in real time to better correct for atmospheric extinction.


1966 ◽  
Vol 12 (2) ◽  
pp. 607-609
Author(s):  
A. H. Cook

The Chairman, W. Fricke, President of Commission 4, opened the Joint Discussion by drawing attention to the purpose and proposed procedure for the meeting. The Joint Discussion had been arranged by the Executive Committee of the Union in order to avoid the necessity for separate discussions by each Commission that was affected by the Report of the Working Group on the IAU System of Astronomical Constants. The Organizing Committee therefore proposed the following resolution:‘The members of the IAU at this Joint Discussion recommend to the Executive Committee that the following resolution be put before the General Assembly: “The International Astronomical Union endorses the final list of constants prepared by the Working Group on the System of Astronomical Constants and recommends that it be used in the national and international astronomical ephemerides at the earliest practicable date.’”


1966 ◽  
Vol 12 (2) ◽  
pp. 604-606
Author(s):  
W. Fricke

The Chairman, W. Fricke, President of Commission 4, opened the Joint Discussion by drawing attention to the purpose and proposed procedure for the meeting. The Joint Discussion had been arranged by the Executive Committee of the Union in order to avoid the necessity for separate discussions by each Commission that was affected by the Report of the Working Group on the IAU System of Astronomical Constants. The Organizing Committee therefore proposed the following resolution:‘The members of the IAU at this Joint Discussion recommend to the Executive Committee that the following resolution be put before the General Assembly: “The International Astronomical Union endorses the final list of constants prepared by the Working Group on the System of Astronomical Constants and recommends that it be used in the national and international astronomical ephemerides at the earliest practicable date.’”


1997 ◽  
Vol 23 (1) ◽  
pp. 59-60
Author(s):  
H. R. Butcher

The idea for a Working Group (WG) on “Future Large Scale Facilities in Astronomy” grew from a discussion held on 20 August, 1994, during the IAU General Assembly in The Hague. The IAU Executive Committee approved its formation in August, 1995, and its composition in October, 1995. The WG will remain active at least until the XXIIIrd General Assembly in Kyoto in 1997. Members are: H. Butcher (Chairman), R. Ekers, B. Fort, N. Kardashev, M. Longair, F. Pacini, L. Rodriguez, G. Swarup, Y. Tanaka, H. Tananbaun, and L. Woltjer (ex officio). The WG carries out its work mostly by email and FAX.


1970 ◽  
Vol 14 (1) ◽  
pp. 123-123
Author(s):  
A. Keith Pierce

Of a select list of about 40 Fraunhofer lines distributed between λλ 3083-7122, central intensities corrected for scattered light, ghosts and instrumental profile, has been obtained for 18 lines. Uncorrected values of central intensity for a number of other lines are available. A complete list of the results of all observers will be given at the General Assembly in Brighton.


1998 ◽  
Vol 37 (2) ◽  
pp. 249-260 ◽  

Recalling its resolution 49/60 of 9 December 1994, by which it adopted the Declaration on Measures to Eliminate International Terrorism, and its resolution 51/210 of 17 December 1996,Having considered the text of the draft convention for the suppression of terrorist bombings prepared by the Ad Hoc Committee established by General Assembly resolution 51/210 of 17 December 1996 1/ and the Working Group of the Sixth Committee, 2/


1973 ◽  
Vol 15 (1) ◽  
pp. 716-716
Author(s):  
B. Hauck

This Group was formed during the meeting of the General Assembly in Brighton on August 22, 1970 with the following members: B. E. Westerlund, W. P. Bidelman, M. Barbier and B. Hauck. In the beginning of 1972 C. O. Jaschek was asked to join this group as he is also a member of the IAU Working Group on Numerical Data.The first work of our Group was to establish a list of catalogues recently published or in preparation. For this purpose a circular letter was sent to all members of our Commission. Dr Crawford, President of Commission 25, kindly sent our letter to the members of his Commission. The first list was published in the ‘Bulletin d'lnformation no. 1 du Centre de Donnees Stellaires de Strasbourg’. A complement has been published in the second issue of this bulletin. We thank all colleagues who have contributed, and we hope that many colleagues will contribute to the success of a second list sending us their information and data.


2000 ◽  
Vol 24 (1) ◽  
pp. 176-185
Author(s):  
Philippe Eenens ◽  
Joseph Cassinelli ◽  
Peter Conti ◽  
Catharine Garmany ◽  
Karel van der Hucht ◽  
...  

The Working Group on Hot Massive Stars has been officially recognized by the IAU Executive Committee during the XXIII General Assembly in August 1997. Its origins are the Hot Star Newsletter, launched in 1994, and a long tradition of interaction and collaborative research strengthened by a series of meetings on hot beaches. It gathers over 500 researchers working on OB stars, Luminous Blue Variables, Wolf-Rayet stars, and in general all topics related to the evolution of massive stars and to the physics and consequences of winds from hot stars. The very successful recent symposium on “Wolf-Rayet phenomena in massive stars and starburst galaxies” is an indicator of the increasing interest of the extragalactic community in the study of these extraordinary stars.


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