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• W2162277752 endingPage "1391" @default.
• W2162277752 startingPage "1372" @default.
• W2162277752 abstract "Using Hα emission as a tracer of ongoing (<16 Myr old) and near-ultraviolet (UV) emission as a tracer of recent (16–100 Myr old) star formation, we present constraints on the properties of core-collapse (CC) supernova (SN) progenitors through the association of their explosion sites with star-forming regions. Amalgamating previous results with those gained from new data, we present statistics of a large sample of SNe; 163.5 Type II (58 IIP, 13 IIL, 13.5 IIb, 19 IIn and 12 ‘impostors’, plus 48 with no sub-type classification) and 96.5 Type Ib/c (39.5 Ib and 52 Ic, plus five with no sub-type classification). Using pixel statistics we build distributions of associations of different SN types with host galaxy star formation. Our main findings and conclusions are as follows. An increasing progenitor mass sequence is observed, implied from an increasing association of SNe to host galaxy Hα emission. This commences with the Type Ia showing the weakest association, followed by the Type II, then the Ib, with the Type Ic showing the strongest correlation to star-forming regions. Thus, our progenitor mass sequence runs Ia—II—Ib—Ic. Overall, the Type Ibc SNe are found to occur nearer to bright H ii regions than SNe of Type II. This implies that the former have shorter stellar lifetimes, thus arising from more massive progenitor stars. While Type IIP SNe do not closely follow the ongoing star formation, they accurately trace the recent formation. This implies that their progenitors arise from stars at the low end of the CC SN mass sequence, consistent with direct detections of progenitors in pre-explosion imaging. Similarly, the Type IIn SNe trace recent but not the ongoing star formation. This implies that, contrary to the general consensus, the majority of these SN do not arise from the most massive stars. Results and suggestive constraints are also presented for the less numerous SNe of Types IIL and IIb, and SN ‘impostors’. Finally, we present an analysis of possible biases in the data, the results of which argue strongly against any selection effects that could explain the relative excess of Type Ibc SNe within bright H ii regions. Thus, intrinsic progenitor differences in the sense of the mass sequence we propose remain the most plausible explanation of our findings." @default.
• W2162277752 created "2016-06-24" @default.
• W2162277752 creator A5001235890 @default.
• W2162277752 creator A5009374040 @default.
• W2162277752 creator A5010598612 @default.
• W2162277752 creator A5011903388 @default.
• W2162277752 date "2012-06-28" @default.
• W2162277752 modified "2023-09-30" @default.
• W2162277752 title "Progenitor mass constraints for core-collapse supernovae from correlations with host galaxy star formation★" @default.
• W2162277752 cites W1619925861 @default.
• W2162277752 cites W1775535351 @default.
• W2162277752 cites W1966699999 @default.
• W2162277752 cites W1970939299 @default.
• W2162277752 cites W1977939445 @default.
• W2162277752 cites W1980907391 @default.
• W2162277752 cites W1982502140 @default.
• W2162277752 cites W1987947934 @default.
• W2162277752 cites W1991506407 @default.
• W2162277752 cites W1996537612 @default.
• W2162277752 cites W2001465642 @default.
• W2162277752 cites W2004570903 @default.
• W2162277752 cites W2005094094 @default.
• W2162277752 cites W2012829886 @default.
• W2162277752 cites W2015295900 @default.
• W2162277752 cites W2015995836 @default.
• W2162277752 cites W2028491290 @default.
• W2162277752 cites W2029254695 @default.
• W2162277752 cites W2035212947 @default.
• W2162277752 cites W2036062947 @default.
• W2162277752 cites W2039450056 @default.
• W2162277752 cites W2044496494 @default.
• W2162277752 cites W2046550784 @default.
• W2162277752 cites W2049500340 @default.
• W2162277752 cites W2050470132 @default.
• W2162277752 cites W2062043857 @default.
• W2162277752 cites W2063453376 @default.
• W2162277752 cites W2064631236 @default.
• W2162277752 cites W2074431966 @default.
• W2162277752 cites W2082987405 @default.
• W2162277752 cites W2084916516 @default.
• W2162277752 cites W2087033679 @default.
• W2162277752 cites W2088668851 @default.
• W2162277752 cites W2090231561 @default.
• W2162277752 cites W2091047626 @default.
• W2162277752 cites W2094018535 @default.
• W2162277752 cites W2096911128 @default.
• W2162277752 cites W2101726256 @default.
• W2162277752 cites W2106827229 @default.
• W2162277752 cites W2108679361 @default.
• W2162277752 cites W2110044294 @default.
• W2162277752 cites W2112986409 @default.
• W2162277752 cites W2117757935 @default.
• W2162277752 cites W2123423036 @default.
• W2162277752 cites W2127569230 @default.
• W2162277752 cites W2130040310 @default.
• W2162277752 cites W2130197607 @default.
• W2162277752 cites W2130275104 @default.
• W2162277752 cites W2136070800 @default.
• W2162277752 cites W2139777473 @default.
• W2162277752 cites W2140594322 @default.
• W2162277752 cites W2141067605 @default.
• W2162277752 cites W2141344482 @default.
• W2162277752 cites W2157990947 @default.
• W2162277752 cites W2160017206 @default.
• W2162277752 cites W2164099233 @default.
• W2162277752 cites W2171521025 @default.
• W2162277752 cites W2328436769 @default.
• W2162277752 cites W2949096495 @default.
• W2162277752 cites W2950346593 @default.
• W2162277752 cites W3091017234 @default.
• W2162277752 cites W3098257731 @default.
• W2162277752 cites W3098636134 @default.
• W2162277752 cites W3098866588 @default.
• W2162277752 cites W3099014370 @default.
• W2162277752 cites W3099257556 @default.
• W2162277752 cites W3099532746 @default.
• W2162277752 cites W3100334026 @default.
• W2162277752 cites W3100783907 @default.
• W2162277752 cites W3100862643 @default.
• W2162277752 cites W3100939102 @default.
• W2162277752 cites W3100961840 @default.
• W2162277752 cites W3101287766 @default.
• W2162277752 cites W3102616519 @default.
• W2162277752 cites W3102864016 @default.
• W2162277752 cites W3103868583 @default.
• W2162277752 cites W3104045763 @default.
• W2162277752 cites W3104145990 @default.
• W2162277752 cites W3104410307 @default.
• W2162277752 cites W3105995737 @default.
• W2162277752 cites W3106160139 @default.
• W2162277752 cites W3121602922 @default.
• W2162277752 cites W3123956260 @default.
• W2162277752 cites W3124032753 @default.
• W2162277752 cites W3124041400 @default.
• W2162277752 cites W4250000592 @default.
• W2162277752 cites W4293417899 @default.
• W2162277752 cites W4295004167 @default.
• W2162277752 cites W4298291642 @default.

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