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ഫലകം:Infobox globular cluster - വിക്കിപീഡിയ
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Infobox for articles on globular clusters.
Fields should generally be directly from the source, such as SIMBAD. Wikilinks and expansion of abbreviations are acceptable.
The following parameters can be used to create a globular cluster infobox. Please remove any parameters that are not likely to be useful.
{{Infobox globular cluster | name = | image = | caption = | credit = | epoch = | class = | constellation = | ra = | dec = | dist_ly = | dist_pc = | appmag_v = | size_v = | mass_msol = | mass_kg = | radius_arcminsec = | radius_ly = | radius_pc = | radius_tidal_arcminsec = | radius_tidal_ly = | radius_tidal_pc = | v_hb = | metal_fe = | age = | notes = | names = }}
Common name of the globular cluster. This field is required.
Photograph of the cluster. Preferably this should be a wide shot to show most/all of the globular cluster rather than a view from within it. Include the "File:" prefix and a width of 300px. If uploading a new image, please put them on Commons so they can be easily used by the other language Wikipedias.
Description of the photograph in the image field.
Credit for the photograph in the image field.
The astronomical epoch of the cluster coordinates (below). Normally this is [[J2000]].
The Shapley–Sawyer Concentration Class of the cluster.
A link to the constellation where this cluster is located.
The right ascension coordinate of the cluster midpoint. The {{RA}} or {{Deg2HMS}} templates should be used here. For example: {{RA|hh|mm|ss.dd}} or {{Deg2HMS|dd.ddd|sup=yes}}.
The declination coordinate of the cluster midpoint. The {{DEC}} template should be used here. For example: {{DEC|±dd|mm|ss.d}}.
This is an estimate of the cluster's distance from the Solar System in light years. The distances can be combined into a single field as: {{Convert|d.dd|kly|kpc|abbr=off|lk=on|sigfig=1}}.
This should be the same distance as dist_ly using parsec as the units. A parsec is equal to 3.2616 light years.
The apparent magnitude of the cluster.
This gives the angular diameter, usually in arc minutes or arc seconds.
The estimated total mass in solar masses.
The same value as above, using kilograms as units. A solar mass is equal to 2 × 1030 kg.
The angle subtended by the radius, in arcminutes or arcseconds.
The ly and pc radii can be combined into a single field as: {{Convert|d.dd|ly|pc|abbr=on|lk=on|sigfig=1}}.
This should be the same distance as radius_ly using parsec as the units. A parsec is equal to 3.2616 light years.
The angle subtended by the tidal radius, in arcminutes or arcseconds (specify).
This is the Roche limit of the cluster, beyond which stars and material are effectively removed from the cluster. Typically given as either the instantaneous value or an average of its perigalactic and apogalactic values.
The ly and pc radii can be combined into a single field as: {{Convert|d.dd|ly|pc|abbr=on|lk=on|sigfig=1}}.
This should be the same distance as radius_tidal_ly using parsec as the units. A parsec is equal to 3.2616 light years.
The visual magnitude of the horizontal branch stars in the cluster.
The metallicity as a logarithmic abundance of iron relative to hydrogen, as compared to the Sun.
The estimated age of the cluster, usually listed in [[Gigayear|Gyr]] (billions of years).
Additional details of significance.
A comma separated list of used alternative cluster names. These are names that are commonly used in scholarly journal articles, such as the New General Catalogue (NGC) name.
മുകളിൽ കാണുന്ന വിവരണം ഫലകം:Infobox globular cluster/doc എന്ന ഉപതാളിൽ നിന്ന് ഉൾപ്പെടുത്തിയിട്ടുള്ളതാണ്. (തിരുത്തുക | നാൾവഴി)
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"https://ml.wikipedia.org/w/index.php?title=ഫലകം:Infobox_globular_cluster&oldid=1467908" എന്ന താളിൽനിന്ന് ശേഖരിച്ചത്
ഈ താൾ അവസാനം തിരുത്തപ്പെട്ടത്: 20:31, 31 ഒക്ടോബർ 2012.
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