What determines the γ-ray luminosities of classical novae?
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| Title: | What determines the γ-ray luminosities of classical novae? |
|---|---|
| Authors: | Craig, Peter1, Aydi, Elias2, Chomiuk, Laura1, Stone, Ashley3, Strader, Jay1, Chong, Atticus1, Li, Kwan-Lok4, Fan, Jhih-Ling4, Bahramian, Arash5, Buckley, David A H6 |
| Source: | Monthly Notices of the Royal Astronomical Society; Mar2026, Vol. 546 Issue 3, p1-54, 54p |
| Database: | Applied Science & Technology Source |
| FullText | Text: Availability: 0 |
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| Header | DbId: aci DbLabel: Applied Science & Technology Source An: 192224821 AccessLevel: 2 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| PLink | https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=aci&AN=192224821 |
| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1093/mnras/staf2270 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 54 StartPage: 1 Titles: – TitleFull: What determines the γ-ray luminosities of classical novae? Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Craig, Peter – PersonEntity: Name: NameFull: Aydi, Elias – PersonEntity: Name: NameFull: Chomiuk, Laura – PersonEntity: Name: NameFull: Stone, Ashley – PersonEntity: Name: NameFull: Strader, Jay – PersonEntity: Name: NameFull: Chong, Atticus – PersonEntity: Name: NameFull: Li, Kwan-Lok – PersonEntity: Name: NameFull: Fan, Jhih-Ling – PersonEntity: Name: NameFull: Bahramian, Arash – PersonEntity: Name: NameFull: Buckley, David A H IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 03 Text: Mar2026 Type: published Y: 2026 Identifiers: – Type: issn-print Value: 00358711 Numbering: – Type: volume Value: 546 – Type: issue Value: 3 Titles: – TitleFull: Monthly Notices of the Royal Astronomical Society Type: main |
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