टेम्पलेट:Infobox supercluster
| {{{name}}} | |
|---|---|
| Observation data (Epoch {{{epoch}}}) | |
| Constellation(s) | {{{constellation}}} |
| Right ascension | {{{ra}}} |
| Declination | {{{dec}}} |
| Brightest member | {{{brightest_member}}} |
| Number of clusters | {{{member_no}}} |
| Major axis | {{{major_axis_mpc}}} |
| Minor axis | {{{minor_axis_mpc}}} |
| Redshift | {{{redshift}}} |
| Distance (co-moving) | {{{distance}}} |
| Binding mass | {{{mass}}} M☉ |
| Luminosity (specify) | {{{luminosity}}} |
| Flux (specify) | {{{flux}}} |
| Other designations | |
| {{{other_names}}} | |
| See also: Galaxy groups, Galaxy clusters, List of superclusters | |
Infobox for articles on superclusters of galaxies. Intended for the creation of new supercluster pages and for updating older pages with outdated infoboxes.
Usage
[संपादन करीं]{{Infobox supercluster
| name =
| image =
| caption =
| credit =
| epoch =
| constellation =
| ra = {{RA|00|00}} or {{Deg2HMS|000.000|sup=yes}}
| dec = {{DEC|±00|00}}
| brightest_member =
| member_no =
| major_axis_mpc = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| minor_axis_mpc = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| redshift =
| distance = {{convert|000|Mpc|Mly|0|abbr=on|lk=on}} {{hub|0.00}}
| mass = 0{{e|14}} {{hub|0.00}} <!-- In solar masses -->
| luminosity = ({{solar luminosity|link=y}}, if applicable)
| flux =
| other_names =
}} |
Parameters
[संपादन करीं]name
[संपादन करीं]<Name of the object> Supercluster, i.e. Shapley Supercluster
image
[संपादन करीं]Associated image of the object: [[Image:name.png|400px]]
caption
[संपादन करीं]Text underneath the image.
credit
[संपादन करीं]To whom do we owe this great pleasure?
epoch
[संपादन करीं]Equatorial coordinates based on which epoch? If other than J2000, please find or convert to J2000.
constellation
[संपादन करीं]Wikilink(s) to constellation(s).
ra
[संपादन करीं]{{RA|00|00}} or {{Deg2HMS|000.000|sup=yes}}
dec
[संपादन करीं]{{DEC|±00|00}}
brightest_member
[संपादन करीं]The brightest cluster.
member_no
[संपादन करीं]The number of galaxy clusters belonging to the supercluster.
major_axis_mpc
[संपादन करीं]The major axis of the supercluster in h−1
, h−1
0.70, h−1
0.75, etc., megaparsecs. See distance section.
minor_axis_mpc
[संपादन करीं]The minor axis of the supercluster in h−1
, h−1
0.70, h−1
0.75, etc., megaparsecs. See distance section.
redshift
[संपादन करीं]- z, if ≳ 0.1 :
0.8 - z (km/s), if ≲ 0.1 :
0.0717 (21 500 km/s)
distance
[संपादन करीं]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 मेगापारसेक (326.16 मेगाप्रकाशवर्ष) h−1
0.73{{convert|100|+/-|20|Mpc|Mly|abbr=on|lk=on}}{{hub|0.73}}gives 100 ± 20 मेगापारसेक (326 ± 65 मेगाप्रकाशवर्ष) 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 scales.
mass
[संपादन करीं]luminosity
[संपादन करीं]Make sure to specify the passband:
- X-ray luminosity is usually given in erg s−1 for some keV range.
- Visible or bolometric luminosity is usually given in L☉.
1.4{{e|14}} {{hub|0.70}} {{solar luminosity|link=y}}gives 1.4×1014 h−1
0.70 L☉
flux
[संपादन करीं]If available, use alternatively to luminosity. Make sure to specify the passband.
other_names
[संपादन करीं]Please don't list all the cross-identifications in NED for each object.