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{{{name}}}
{{{image}}}

Zasluge: {{{credit}}}
Opazovalni podatki (epoha {{{epoch}}})
Ozvezdje{{{constellation}}}
Rektascenzija{{{ra}}}
Deklinacija{{{dec}}}
Najsvetlejša članica{{{brightest member}}}
Število galaksij{{{member no}}}
Razred količine galaksij{{{richness}}}
Bautz-Morganova razvrstitev{{{bmtype}}}
Hitrost širjenja{{{velocity dispersion}}}
Rdeči premik{{{redshift}}}
Oddaljenost
(co-moving)
{{{distance}}}
Temperatura medgalaktične snovi{{{temperature}}}
Vezalna masa{{{mass}}}
Izsev žarkov X{{{luminosity}}}
Tok žarkov X{{{flux}}}
Druga imena in oznake
{{{other names}}}
Glej tudi: skupine galaksij, jate galaksij
Documentation icon Dokumentacija predloge[predogled] [uredi] [zgodovina] [osveži]

Infopolje za člank o skupinah in jatah galaksij.

UporabaUredi

{{Infopolje jata galaksij
| name = 
| image = 
| caption = 
| credit = 
| epoch = 
| constellation = 
| ra = {{RA|00|00}}
| dec = {{DEC|±00|00}}
| brightest_member = 
| member_no = 
| richness = 
| bmtype = 
| velocity_dispersion = 
| redshift = 
| distance = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0,00}}
| temperature = 
| mass = 0{{e|14}} {{hub|0.00}} [[sončeva masa|M<sub>☉</sub>]]
| luminosity = 
| flux = 
| other_names = 
}}



ParametriUredi

nameUredi

Ime objekta wikipovezanega na stran o katalogu, t.j. Abell 370, NGC 7318, itd.

imageUredi

Slika objekta: [[Slika:name.png|300px]]

captionUredi

Besedilo pod sliko.

creditUredi

Komu dolgujemo zaslugo?

epochUredi

Equatorial coordinates based on which epoch? If other than J2000, please find or convert to J2000.

constellationUredi

Wikipovezava na ozvezdje.

raUredi

{{RA|00|00}}

decUredi

{{DEC|±00|00}}

brightest_memberUredi

The brightest (visible) member.

member_noUredi

The number of galaxies belonging to the cluster, out to (at least) the virial radius.

richnessUredi

Abell (or related) richness class. Based on number of members within a magnitude range of m3 to m3+2, where m3 is the magnitude of the third brightest member of the cluster. Not to be mistaken for the total number of galaxies in the cluster. Link to the digital version of the entire Abell Catalog is here.

bmtypeUredi

Bautz-Morganova klasifikacija type is available via NASA Extragalactic Database (NED) or the digital version of the Abell Catalog.

velocity_dispersionUredi

Hitrost širjenja of the cluster (as opposed to of only the core).

redshiftUredi

  • z, if ≳ 0,2 : 0,8
  • z (km/s), if ≲ 0,2 : 0,0717 (21 500 km/s)

distanceUredi

NED's default value for the dimensionless Hubble parameter is 0,73 using the WMAP 3-year results, but one is able to change this to match the WMAP 5-year results with h=0,705.

  • If measurement is left in 'units' of h: {{hub|}} gives h−1
  • If h=0,73 is used: {{hub|0,73}} gives h−1
    0,73
  • {{convert|100|Mpc|Mly|2|abbr=on|lk=on}} {{hub|0,73}} gives 100 Mpc (326,16 Mly) h−1
    0,73
  • {{convert|100|+/-|20|Mpc|Mly|abbr=on|lk=on}} {{hub|0,73}} gives 100 ± 20 Mpc (326 ± 65 Mly) h−1
    0,73
  • Use Gpc as appropriate and/or feel free to leave off the light-year conversion if it becomes unwieldy. Parsecs are less ambiguous and are preferred over light-years, especially at cosmological distances (and also at nearby distances were parallaxes can be measured).

temperatureUredi

X-ray temperature of the intracluster medium, usually given in keV.

massUredi

  • 1,4{{e|14}} {{hub|0,70}} [[sončeva masa|M<sub>☉</sub>]] gives 1,4 · 1014 h−1
    0.70
    M

luminosityUredi

  • X-ray luminosity, usually given in erg s-1 for some keV range.
  • 1,4{{e|14}} [[erg]] s<sup>-1</sup> (0,1—2,4 [[Elektronvolt|keV]]) gives 1,4 · 1014 erg s-1 (0,1—2,4 keV)

fluxUredi

  • X-ray flux, usually given in erg s-1 cm-2 for some keV range.
  • (1,4 ± 0,2){{e|-11}} [[erg]] s<sup>-1</sup> cm<sup>-2</sup> (0,1—2,4 [[Elektronvolt|keV]]) gives (1,4 ± 0,2) · 10-11 erg s-1 cm-2 (0,1—2,4 keV)

other_namesUredi

Please don't list all the cross-identifications in NED for each object.

Glej tudiUredi

External linksUredi