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from IPython.display import HTML
from IPython.display import Image
import os
%pylab
%matplotlib inline
%run ../../../utils/load_notebook.py
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from photometry import *
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from instabilities import *
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name = 'N4258'
gtype = 'SA(s)ab'
incl = 70. #(adopted by Epinat+2008)
scale = 0.092 #kpc/arcsec according to ApJ 142 145(31pp) 2011
data_path = '../../data/ngc4258'
sin_i, cos_i = np.sin(incl*np.pi/180.), np.cos(incl*np.pi/180.)
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os.chdir(data_path)
# Данные из NED
HTML('<iframe src=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=ngc+4258&extend=no&hconst=\
73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=\
30000.0&list_limit=5&img_stamp=YES width=1000 height=350></iframe>')
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# Данные из HYPERLEDA
HTML('<iframe src=http://leda.univ-lyon1.fr/ledacat.cgi?o=ngc4258 width=1000 height=350></iframe>')
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#SDSS
Image('ngc3898_SDSS.jpeg', width=300)
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#JHK
Image('ngc3898_JHK.jpg', width=300)
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Дисперсии скоростей и кривая вращения - есть в http://adsabs.harvard.edu/cgi-bin/bib_query?1998A%26AS..133..317H до ~ 50'' (1 разрез)
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Image('u7353.png')
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Кривая вращения:
$\Sigma_{HI}$ и $\Sigma_{H_2}$ https://arxiv.org/pdf/1608.06735v1.pdf
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Image()
$\rm{H_{\alpha}}$, $UV$