Документ взят из кэша поисковой машины. Адрес оригинального документа : http://hea-www.harvard.edu/ChandraSNR/G042.8+00.6/1954/work/main.info Дата изменения: Mon Aug 15 22:12:34 2005 Дата индексирования: Tue Oct 2 11:31:08 2012 Кодировка: Поисковые слова: http astrokuban.info astrokuban

snr_name=G042.8+00.6
common_name=SGR 1900+14

#distance in kpc(eg. 50)
distance=6

#note on distance
distance_note= \cite{Hurley1999}

#1 if remnant has central source
has_central_source=1

#1 if it has pulsar nebula page
pulsar_nebular_page=0
link_to_green=http:

#position of of central source. unit in degree.(eg. 85.04, -69.3)
#get it from "size.reg"
central_source_ra=286.8092917
central_source_dec=9.3225278

#position of of x-ray center. unit in degree.(eg. 85.04, -69.3)
#and its size(free format)
#get it from "size.reg"
xray_center_ra=286.8092917
xray_center_dec=9.3225278
xray_size=pt source
xray_flux=

#description of remnant
description=bright SGR located well outside shell of remnant

#path to image on far right
top_image1=1983/work/tr2.jpg
#path to image
top_image2=

#not on chip. will be placed in observation section.
#eg. whole remnant are within chip S3(C7)
#eg. pile up and trailed image due to high count rate of pulsar
#eg. \cite{g_caveat_pileup} and \cite{g_caveat_trailedimage}
#just add more if you need more (eg. summary_note04=..)
summary_note01=not clear if SGR and remnant are associated
summary_note02=SGR is outside shell of remnant
summary_note03=Spectrum is distorted by pileup

#note on fitting procedure.
#eg. Two Plane Parallel Shock model for shell and Power law for central pulsar
fit_note01=Pileup model used to correct spectrum but index probably uncertain.