Integrative Levels Classification

ILC edition 2
Expanded class `hl`

▽ ⌕ `hɭ` /ɣala/	stars ↞ `gf` plasma ✍
▽ ⌕ `hɭ91` /ɣalaɲɔmpɔ/ `[bpa]`	at evolutionary stage
▽ ⌕ `hɭ91k` /ɣalaɲɔmpɔka/	protostars
▽ ⌕ `hɭ91n` /ɣalaɲɔmpɔna/	young stellar objects
▽ ⌕ `hɭ91p` /ɣalaɲɔmpɔpa/	main sequence stars
▽ ⌕ `hɭ91q` /ɣalaɲɔmpɔca/	neutron stars
▽ ⌕ `hɭ95` /ɣalaɲɔlpɔ/ `[hla]`	undergoing star process
▽ ⌕ `hɭ99` /ɣalaɲɔɲɔ/ `[hlat]`	spectral type
▽ ⌕ `hɭU` /ɣaluj/	the Sun ↞ `hld` dwarf stars `hl91n` young stellar objects
▽ ⌕ `hɭan` /ɣalɛna/	stellar nucleosynthesis
▽ ⌕ `hɭat` /ɣalɛta/	spectral types
▽ ⌕ `hɭatb` /ɣalɛtaba/	O; blue
▽ ⌕ `hɭatc` /ɣalɛtaʃa/	B; blue white
▽ ⌕ `hɭate` /ɣalɛte/	A; white
▽ ⌕ `hɭatf` /ɣalɛtafa/	F; yellow white
▽ ⌕ `hɭatg` /ɣalɛtaga/	G; yellow
▽ ⌕ `hɭatk` /ɣalɛtaka/	K; orange
▽ ⌕ `hɭatm` /ɣalɛtama/	M; red
▽ ⌕ `hɭatr` /ɣalɛtara/	L
▽ ⌕ `hɭatt` /ɣalɛtata/	T
▽ ⌕ `hɭb` /ɣalaba/	subdwarf stars
▽ ⌕ `hɭd` /ɣalada/	dwarf stars
▽ ⌕ `hɭf` /ɣalafa/	subgiant stars
▽ ⌕ `hɭg` /ɣalaga/	giant stars
▽ ⌕ `hɭh` /ɣalaɣa/	bright giant stars
▽ ⌕ `hɭj` /ɣalaʒa/	supergiant stars
▽ ⌕ `hɭk` /ɣalaka/	hypergiant stars
Connected classes:
▽ ⌕ `hɭ95` `[hla]`	undergoing star process
▽ ⌕ `hɭ99` `[hlat]`	spectral type
▽ ⌕ `hɭU`	the Sun ↞ `hld hl91n`
▽ ⌕ `hpU`	solar planets ↞ `hlU`
▽ ⌕ `hqdU`	solar dwarf planets ↞ `hlU`
▽ ⌕ `hqn`	centaurs ↞ `hlU`
▽ ⌕ `htU`	the Solar system ↞ `hlU`
▽ ⌕ `hu`	star clusters; stellar clusters ↞ `hl`
▽ ⌕ `vahv`	solar technology ↞ `hlU`

specificity
current: 99

Move to another main class:
a b c d e f g h i j k l m n o p q r s t u v w x y


Facets key
0  as for perspective 
1  at time            
2  in place           
3  by agent           
4  despite disorder   
5  with transformation
6  having property    
7  with part          
8  as form            
9  of kind

ILC edition 2. Expanded class hl / — ISKO Italia <http://www.iskoi.org/ilc/2/no.php?no=hl> : 2019.09.18 - 2019.10.22 -

ILC edition 2Expanded class hl

ILC edition 2
Expanded class `hl`