Brandt, Søren

Castro-Tirado, A. J.

Lund, Niels

Online Research Database In Technology

                       General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights.  • Users may download and print one copy of any publication from the public portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain • You may freely distribute the URL identifying the publication in the public portal   If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim.     Downloaded from orbit.dtu.dk on: Dec 20, 20174U 0614+09Brandt, Søren; Lund, Niels; Castro-Tirado, A. J.Published in:International Astronomical Union Circulars (IAUC)Publication date:1993Document VersionPublisher's PDF, also known as Version of recordLink back to DTU OrbitCitation (APA):Brandt, S., Lund, N., & Castro-Tirado, A. J. (1993). 4U 0614+09. International Astronomical Union Circulars(IAUC), (5710).                                                  Circular No. 5710 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM     EASYLINK 62794505 MARSDEN@CFA or GREEN@CFA (.SPAN, .BITNET or .HARVARD.EDU)  4U 0614+09      S. Brandt, N. Lund and A. J. Castro-Tirado, Danish Space Research Institute, report: "An x-ray burst from the low-mass x-ray binary 4U 0614+09 has been detected by the WATCH all-sky monitor on the EURECA satellite.  The burst started on Feb. 17.46513 UT and in eight seconds reached a peak flux of 15 Crab in the 6-15-keV energy band.  The flux decayed with an e-folding time of about 15 seconds."  1993 BW2      Further precise positions have been reported as follows:       1993 UT             R.A. (2000) Decl.       Observer      Feb.  2.98084    6 44 00.54   +39 58 44.4   Bendjoya            2.98582    6 44 01.09   +39 59 03.3     "            2.98848    6 44 01.44   +39 59 14.2     "           18.14792    7 16 57.67   +49 45 49.9   McCrosky           18.15744    7 16 58.86   +49 45 59.8     "  P. Bendjoya and A. Maury (Observatoire de la Cote d'Azur).  0.9-m CERGA    Schmidt + CCD.  Reduction by Maury and J. B. Edmond. R. E. McCrosky and C.-Y. Shao (Oak Ridge).  1.5-m reflector + CCD.       Improved orbital elements from 12 observations Jan. 28-Feb. 18:       T = 1992 Nov. 20.1158 TT         Peri. = 287.2101      e = 0.304419                     Node  = 121.2250  2000.0      q = 0.926126 AU                  Incl. =  21.8299        a =  1.331442 AU    n = 0.6415352    P =   1.536 years  1993 TT     R. A. (2000) Decl.     Delta      r    Elong. Phase      V Feb. 17     7 14.43    +49 23.6    0.323    1.218  129.1   39.0     17.0      22     7 25.56    +50 43.8    0.369    1.242  125.8   40.2     17.4      27     7 36.87    +51 28.9    0.416    1.266  122.9   41.1     17.7 Mar.  4     7 48.32    +51 48.0    0.465    1.289  120.1   41.7     18.0       9     7 59.84    +51 47.3    0.514    1.312  117.6   42.1     18.3      14     8 11.35    +51 31.1    0.564    1.335  115.1   42.4     18.5      19     8 22.84    +51 02.3    0.614    1.357  112.8   42.5     18.8      24     8 34.28    +50 23.1    0.666    1.379  110.5   42.6     19.0  1993 February 18               (5710)              Brian G. Marsden 

4U 0614+09

http://orbit.dtu.dk/ws/files/52280639/IAU_Circular_5710_1993.pdf

4U 0614+09

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