See Hayashi track on Wiktionary
{
"head_templates": [
{
"args": {
"1": "?"
},
"expansion": "Hayashi track",
"name": "en-noun"
}
],
"lang": "English",
"lang_code": "en",
"pos": "noun",
"senses": [
{
"categories": [
{
"kind": "other",
"name": "English entries with incorrect language header",
"parents": [
"Entries with incorrect language header",
"Entry maintenance"
],
"source": "w"
},
{
"kind": "other",
"name": "Pages with 1 entry",
"parents": [],
"source": "w"
},
{
"kind": "other",
"name": "Pages with entries",
"parents": [],
"source": "w"
},
{
"kind": "topical",
"langcode": "en",
"name": "Astrophysics",
"orig": "en:Astrophysics",
"parents": [
"Astronomy",
"Physics",
"Sciences",
"Space",
"All topics",
"Nature",
"Fundamental"
],
"source": "w"
}
],
"glosses": [
"A luminosity–temperature relationship obeyed by infant stars of less than 3 M☉ in the pre-main-sequence phase (PMS phase) of stellar evolution."
],
"id": "en-Hayashi_track-en-noun-eKrlzlue",
"links": [
[
"astrophysics",
"astrophysics"
],
[
"luminosity",
"luminosity"
],
[
"temperature",
"temperature"
],
[
"relationship",
"relationship"
],
[
"obey",
"obey"
],
[
"infant",
"infant"
],
[
"stars",
"stars"
],
[
"M☉",
"M☉"
],
[
"stellar",
"stellar"
],
[
"evolution",
"evolution"
]
],
"raw_glosses": [
"(astrophysics) A luminosity–temperature relationship obeyed by infant stars of less than 3 M☉ in the pre-main-sequence phase (PMS phase) of stellar evolution."
],
"topics": [
"astrophysics"
]
}
],
"word": "Hayashi track"
}
{
"head_templates": [
{
"args": {
"1": "?"
},
"expansion": "Hayashi track",
"name": "en-noun"
}
],
"lang": "English",
"lang_code": "en",
"pos": "noun",
"senses": [
{
"categories": [
"English countable nouns",
"English entries with incorrect language header",
"English lemmas",
"English multiword terms",
"English nouns",
"English nouns with unknown or uncertain plurals",
"Pages with 1 entry",
"Pages with entries",
"en:Astrophysics"
],
"glosses": [
"A luminosity–temperature relationship obeyed by infant stars of less than 3 M☉ in the pre-main-sequence phase (PMS phase) of stellar evolution."
],
"links": [
[
"astrophysics",
"astrophysics"
],
[
"luminosity",
"luminosity"
],
[
"temperature",
"temperature"
],
[
"relationship",
"relationship"
],
[
"obey",
"obey"
],
[
"infant",
"infant"
],
[
"stars",
"stars"
],
[
"M☉",
"M☉"
],
[
"stellar",
"stellar"
],
[
"evolution",
"evolution"
]
],
"raw_glosses": [
"(astrophysics) A luminosity–temperature relationship obeyed by infant stars of less than 3 M☉ in the pre-main-sequence phase (PMS phase) of stellar evolution."
],
"topics": [
"astrophysics"
]
}
],
"word": "Hayashi track"
}
Download raw JSONL data for Hayashi track meaning in All languages combined (1.1kB)
This page is a part of the kaikki.org machine-readable All languages combined dictionary. This dictionary is based on structured data extracted on 2025-03-01 from the enwiktionary dump dated 2025-02-21 using wiktextract (7c21d10 and f2e72e5). The data shown on this site has been post-processed and various details (e.g., extra categories) removed, some information disambiguated, and additional data merged from other sources. See the raw data download page for the unprocessed wiktextract data.
If you use this data in academic research, please cite Tatu Ylonen: Wiktextract: Wiktionary as Machine-Readable Structured Data, Proceedings of the 13th Conference on Language Resources and Evaluation (LREC), pp. 1317-1325, Marseille, 20-25 June 2022. Linking to the relevant page(s) under https://kaikki.org would also be greatly appreciated.