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Базовые свойства галактик местного объема (

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Рисунок 1.1. Продолжение.

Приложение B Таблица 1. Список пользовательских функций.

SELECT

CASE KD

morphology.t::double precision = 0::double precision THEN 0.081::double (Fouque&Paturel 1985)

SELECT

FROM morphology WHERE morphology.id=($1) AND morphology.preferable;

SELECT

cz.cz + 316::double precision * (sin(radians(objects.b)) * sin(radians(- адиортнец оньлетисонто 4::double precision)) + cos(radians(objects.b)) * cos(radians(- 4::double ыппург йонтсеМ precision)) * cos(radians(objects.l - 93::double precision))) LEFT JOIN cz ON cz.id=$1 AND cz.preferable WHERE objects.id=$1;

SELECT

morphology.t::double precision = 10::double precision THEN 10::double апит огоксечиголофром morphology.t::double precision = 8::double precision THEN 10::double precision ^ ((- 0.43::double precision) - 0.053::double precision * morphology.t::double precision) FROM morphology WHERE morphology.id=$1 AND morphology.preferable;

SELECT sqrt(GREATEST(25::double precision, precision*((hiwidth.w/(1::double precision + cal_z($1)))/120.0::double и укварпоп precision*((hiwidth.w/(1::double precision + cal_z($1)))/120.0::double precision)^2::double precision)))) FROM hiwidth WHERE hiwidth.id=$1 AND hiwidth.preferable;

SELECT

WHEN distance.modulus IS NOT NULL THEN 10::double precision ^ (0.2::double precision * distance.modulus - 5::double precision) cal_vlg($1)/get_const('Ho')

ELSE NULL

LEFT JOIN distance ON distance.id=objects.id AND preferable

SELECT

LEAST(1::double precision, sqrt((1::double precision axis_ratio.b_a::double precision ^ 2.0::double precision)) / (1::double precision - (cal_ba0($1) ^ 2.0::double precision)))) FROM axis_ratio WHERE axis_ratio.id=$1 AND axis_ratio.preferable;

SELECT diameter.a*axis_ratio.b_a^0.04::double precision*10.0::double WHERE diameter.id=$1 AND diameter."level" = 26.5::double precision AND еоксечиткалаГ

SELECT

2::double precision*cal_dist($1)*tan((radians(cal_ac($1)/60.0::double артемаид огонйенил в precision))/2.0::double precision)*10.0::double precision^3.0::double асуидар халедерп

SELECT

cal_w50c($1)/(2.0::double precision*sin(radians(cal_incl($1)))); итсорокс йоньлетащарв SELECT GREATEST(0.0::double precision,

SELECT

SELECT

precision*cal_dist($1)^2.0::double precision*get_flux($1,$2) END;

SELECT CASE

SELECT

SELECT

SELECT

SELECT

precision*cal_fluxha_c($1,$2)*cal_dist($1)^2.0::double precision*10::double precision - 0.4::double precision*cal_mag_c($1,$2) + 2.0::double

SELECT

SELECT

cal_mag_c($1,'B')+5::double precision*log(cal_ac($1)) + 8.63::double итсокря йонтсонхревоп

SELECT

cal_dist($1)*cos(radians(objects.decl))*cos(radians(objects.ra*15.0::double аткеъбо танидроок

SELECT

cal_dist($1)*cos(radians(objects.decl))*sin(radians(objects.ra*15.0::double аткеъбо танидроок

SELECT

SELECT

SELECT

precision*cal_mass($1,'HI')/(cal_sfr($1,$2)*get_const('T'))) (Karachentsev&Kaisin Таблица 2. Каталог ближайших галактик.

Таблица3. Вычисляемые параметры ближайших галактик.

Таблица 4. Параметры ближайших галактик, характеризующие активность текущего звездообразования в галактиках.

HIPASSJ0801-21 10 -12.77 -3.59 -0.81 1. Таблица 5. Свиты близких гигантских галактик.



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