Low-metallicity inhibition of type Ia supernovae and galactic and cosmic chemical evolution

scientific article published in January 1998

Low-metallicity inhibition of type Ia supernovae and galactic and cosmic chemical evolution is …
instance of (P31):
scholarly articleQ13442814

External links are
P819ADS bibcode1998ApJ...503L.155K
P818arXiv IDastro-ph/9806335
P356DOI10.1086/311556
P953full work available at URLhttps://iopscience.iop.org/article/10.1086/311556/pdf

P50authorIzumi HachisuQ54165440
P2093author name stringTsujimoto T.
Kato M.
Nomoto K.
Kobayashi C.
P407language of work or nameEnglishQ1860
P304page(s)155–160
P577publication date1998-01-01
P1433published inThe Astrophysical Journal LettersQ3470990
P1476titleLow-metallicity inhibition of type Ia supernovae and galactic and cosmic chemical evolution
P478volume503

Reverse relations

cites work (P2860)
Q68511806Extended star formation in dwarf spheroidal galaxies: The cases of Draco, Sextans, and Ursa Minor
Q56489794Is there an Indication of Evolution of Type [CLC]Ia[/CLC] Supernovae from their Rise Times?
Q56477346Locations of peculiar supernovae as a diagnostic of their origins
Q57828406Nearby Supernova Factory Observations of SN 2005gj: Another Type Ia Supernova in a Massive Circumstellar Envelope
Q56061224New Constraints on ΩM, ΩΛ, and w from an Independent Set of 11 High‐Redshift Supernovae Observed with the Hubble Space Telescope
Q58908406TYPE Ia SUPERNOVA RATE MEASUREMENTS TO REDSHIFT 2.5 FROM CANDELS: SEARCHING FOR PROMPT EXPLOSIONS IN THE EARLY UNIVERSE
Q58474523The Hubble Higher z Supernova Search: Supernovae to z≈ 1.6 and Constraints on Type Ia Progenitor Models
Q59750430The effect of progenitor age and metallicity on luminosity and ^56^Ni yield in type Ia supernovae
Q60522855The most metal-poor damped Lyman $\mathsf{\alpha}$ system at z $\mathsf{<3}$: constraints on early nucleosynthesis
Q56169318X-ray evidence for spectroscopic diversity of type Ia supernovae: XMM observation of the elemental abundance pattern in M87
Q68311590Yields of massive stars and their role in galactic chemical evolution studies