الگو:Infobox globular cluster/توضیحات

از ویکی‌پدیا، دانشنامهٔ آزاد

Infobox for articles on خوشه ستاره‌ای کرویs.

Usage[ویرایش]

Fields should generally be directly from the source, such as سیمباد. Wikilinks and expansion of abbreviations are acceptable.

Example infobox[ویرایش]

{{{Name}}}
{{{image}}}
{{{caption}}}
تولیدکننده: {{{Credit}}}
داده‌های رصدی ({{{epoch}}} مبدأ)
Class{{{درجه}}}
صورت فلکی{{{constellation}}}
بعد (ستاره‌شناسی){{{ra}}}
میل (ستاره‌شناسی){{{dec}}}
نردبان فاصله کیهانی{{{dist_ly}}} ({{{dist_pc}}})
قدر ظاهری (V){{{appmag_v}}}
ابعاد ظاهری (V){{{size_v}}}
ویژگی‌های فیزیکی
جِرم{{{mass_msol}}} M ({{{mass_kg}}} kg)
شعاع{{{radius_arcminsec}}} or {{{radius_ly}}} ({{{radius_pc}}})
حد روش{{{radius_tidal_arcminsec}}} or {{{radius_tidal_ly}}} ({{{radius_tidal_pc}}})
VHB{{{v_hb}}}
فلزیگی{{{metal_fe}}} لگاریتم اعشاری
عمر تخمینی{{{Age}}}
ویژگی‌های شاخص{{{notes}}}
دیگر نام‌ها{{{names}}}
جستارهای وابسته: خوشه ستاره‌ای کروی، فهرست خوشه‌های ستاره‌ای کروی

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 =
| metal_z =
| age =
| notes =
| names =
}}

Parameter documentation[ویرایش]

Field Description
name Common name of the globular cluster. This field is required.
image 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 انبار ویکی‌مدیا so they can be easily used by the other language Wikipedias.
caption Description of the photograph in the image field.
credit Credit for the photograph in the image field.
epoch The astronomical epoch of the cluster coordinates (below). Normally this is [[مبدأ (ستاره‌شناسی)]].
class The Shapley–Sawyer Concentration Class of the cluster.
constellation A link to the صورت فلکی where this cluster is located.
ra The بعد (ستاره‌شناسی) 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}}.
dec The میل (ستاره‌شناسی) coordinate of the cluster midpoint. The {{DEC}} template should be used here. For example: {{DEC|±dd|mm|ss.d}}.
dist_ly 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}}.
dist_pc This should be the same distance as dist_ly using پارسک as the units. A parsec is equal to 3.2616 light years.
appmag_v The قدر ظاهری of the cluster.
size_v This gives the angular diameter, usually in arc minutes or arc seconds.
mass_msol The estimated total mass in جرم خورشیدیes.
mass_kg The same value as above, using kilograms as units. A solar mass is equal to 2 × 1030 kg.
radius_arcminsec The angle subtended by the radius, in arcminutes or arcseconds.
radius_ly The ly and pc radii can be combined into a single field as: {{Convert|d.dd|ly|pc|abbr=on|lk=on|sigfig=1}}.
radius_pc This should be the same distance as radius_ly using پارسک as the units. A parsec is equal to 3.2616 light years.
radius_tidal_arcminsec The angle subtended by the tidal radius, in arcminutes or arcseconds (specify).
radius_tidal_ly This is the حد روش 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}}.

radius_tidal_pc This should be the same distance as radius_tidal_ly using پارسک as the units. A parsec is equal to 3.2616 light years.
v_hb The visual magnitude of the شاخه افقی stars in the cluster.
metal_fe The فلزیگی as a logarithmic abundance of آهن relative to هیدروژن، as compared to the Sun.
metal_z The فلزیگی as a logarithmic abundance of elements other than هیدروژن and هلیم، relative to hydrogen, as compared to the Sun.
age The estimated age of the cluster, usually listed in [[Gigayear|Gyr]] (billions of years).
notes Additional details of significance.
names A comma separated list of used alternative cluster names. These are names that are commonly used in scholarly journal articles, such as the کاتالوگ عمومی جدید (NGC) name.

جستارهای وابسته[ویرایش]