期刊
ASTROPHYSICAL JOURNAL
卷 732, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/732/2/118
关键词
supernovae: general; supernovae: individual (PTF09dav)
资金
- Royal Society
- Einstein fellowship
- NASA
- National Science Foundation [PHY 05-51164, AST 07-07633]
- Gary and Cynthia Bengier
- Richard and Rhoda Goldman Foundation
- W. M. Keck Foundation
- Israeli Science Foundation
- Binational Science Foundation (BSF)
- Weizmann-UK
- EU/FP7 Marie Curie IRG fellowship
- Peter Award
- Patricia Gruber Award
- STFC [ST/G004331/1, ST/I003673/1, ST/H000704/1, ST/H002456/1, PP/E003427/1] Funding Source: UKRI
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1009987] Funding Source: National Science Foundation
- Science and Technology Facilities Council [ST/G004331/1, ST/I003673/1, ST/H000704/1, PP/E003427/1, ST/H002456/1] Funding Source: researchfish
PTF 09dav is a peculiar subluminous Type Ia supernova (SN) discovered by the Palomar Transient Factory (PTF). Spectroscopically, it appears superficially similar to the class of subluminous SN1991bg-like SNe, but it has several unusual features which make it stand out from this population. Its peak luminosity is fainter than any previously discovered SN1991bg-like SN Ia (M-B similar to -15.5), but without the unusually red optical colors expected if the faint luminosity were due to extinction. The photospheric optical spectra have very unusual strong lines of Sc II and Mg I, with possible Sr ii, together with stronger than average Ti ii and low velocities of similar to 6000 km s(-1). The host galaxy of PTF09dav is ambiguous. The SN lies either on the extreme outskirts (similar to 41 kpc) of a spiral galaxy or in an very faint (M-R >= -12.8) dwarf galaxy, unlike other 1991bg-like SNe which are invariably associated with massive, old stellar populations. PTF 09dav is also an outlier on the light-curve-width-luminosity and color-luminosity relations derived for other subluminous SNe Ia. The inferred Ni-56 mass is small (0.019 +/- 0.003 M-circle dot), as is the estimated ejecta mass of 0.36 M-circle dot. Taken together, these properties make PTF 09dav a remarkable event. We discuss various physical models that could explain PTF 09dav. Helium shell detonation or deflagration on the surface of a CO white dwarf can explain some of the features of PTF 09dav, including the presence of Sc and the low photospheric velocities, but the observed Si and Mg are not predicted to be very abundant in these models. We conclude that no single model is currently capable of explaining all of the observed signatures of PTF 09dav.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据