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We present deep, nebular-phase spectropolarimetry of the Type II-P/L SN 2013ej, obtained 167 days after explosion with the European Southern Observatory’s Very Large Telescope. The polarized flux spectrum appears as a nearly perfect (92% correlation), redshifted (by ∼4000 km s⁻¹) replica of the total flux spectrum. Such a striking correspondence has never been observed before in nebular-phase supernova spectropolarimetry, although data capable of revealing it have heretofore been only rarely obtained. Through comparison with 2D polarized radiative transfer simulations of stellar explosions, we demonstrate that localized ionization produced by the decay of a high-velocity, spatially confined clump of radioactive⁵⁶Ni—synthesized by and launched as part of the explosion with final radial velocity exceeding 4500 km s⁻¹—can reproduce the observations through enhanced electron scattering. Additional data taken earlier in the nebular phase (day 134) yield a similarly strong correlation (84%) and redshift, whereas photospheric-phase epochs that sample days 8 through 97 do not. This suggests that the primary polarization signatures of the high-velocity scattering source only come to dominate once the thick, initially opaque hydrogen envelope has turned sufficiently transparent. This detection in an otherwise fairly typical core-collapse supernova adds to the growing body of evidence supporting strong asymmetries across nature’s most common types of stellar explosions, and establishes the power of polarized flux—and the specific information encoded by it in line photons at nebular epochs—as a vital tool in such investigations going forward.

 

Anthropogenic disturbances associated with urban ecosystems can create favorable conditions for populations of some invasive plant species. Light pollution is one of these disturbances, but how it affects the growth and establishment of invasive plant populations is unknown. Cheatgrass (Bromus tectorum) is a problematic invasive species where it has displaced native grassland communities in the United States, but to our knowledge, there have been no studies of the ecological factors that affect cheatgrass presence in urban ecosystems. We conducted field surveys in urban alleys in Denver, Colorado, to compare the presence of cheatgrass at sites with and without artificial light at night (hereafter artificial light) from streetlights. These streetlights are mounted on utility poles, which cause ground disturbance when installed in alleys; we were able to test the independent effect of poles on cheatgrass establishment because not all poles have streetlights on them. We found that cheatgrass was positively associated with the presence of streetlights and to a lesser extent poles. In addition to cheatgrass, we also found that other plants were positively associated with the presence of both poles and streetlights. Our results suggest that artificial light may benefit the occurrence of cheatgrass and other plant species in urban settings. While invasive populations of cheatgrass in wild habitats attract the most attention from managers, we suggest more consideration for this grass in urban environments where its growth and establishment benefit from anthropogenic changes. 

Polarized emission and absorption lines in core-collapse supernovae (CCSNe) trace detailed structures in the ejecta and surrounding circumstellar medium (CSM) that contain clues to the end stages of their progenitors’ lives as massive stars. Extracting this geometrical information, however, requires careful computational modeling that takes into account the 3-D distribution of the ejecta and CSM and the potentially polarizing nature of line scattering. I present the results of such modeling for several CCSNe with multi-epoch polarization observations obtained by the Supernova Spectropolarimetry Project with the SPOL spectropolarimeter. In the cases of “interacting supernovae,” time-variable line polarization can constrain the shape and density of the surrounding CSM, yielding valuable information about the progenitor’s late-stage mass loss episodes. In stripped-envelope supernovae, it provides new, quantitative evidence for the asymmetric nature of the explosions and the possible role of binary companions in shaping the supernova ejecta. 

Supernovae of Type IIb (SNe IIb) are relatively rare events, constituting roughly 10% of all core-collapse supernovae. However, comparative optical spectroscopy of core-collapse events suggest that SNe IIb represent an important transition from the SNe II to SNe Ib sub-type. SNe IIb progenitors are thought to have been stripped of most, but not all, of their hydrogen envelopes by stellar winds or mass transfer in binary systems. Thus, they provide an opportunity to study the effects of mass-loss on stellar evolution. Spectropolarization signatures of these SNe can provide unique information on the spatial distribution of their ejecta and circumstellar environment/interaction. We present multi-epoch spectropolarimetry of SNe IIb selected from the database of the SNSPOL. The observations were obtained using the SPOL instrument at the University of Arizona telescopes. We analyze the time-dependent spectropolarimetric signatures of the objects in this sample and discuss what these imply about the evolution of the overall geometrical structure of the ejecta and circumstellar material in SNe IIb. These time-dependent "snapshots" provide an important window into stripped-envelope SNe and provide further clues regarding the relationship between SNe IIb and other SNe sub-types. 

ABSTRACT We present photometry, spectra, and spectropolarimetry of supernova (SN) 2014ab, obtained through ∼200 d after peak brightness. SN 2014ab was a luminous Type IIn SN (MV < −19.14 mag) discovered after peak brightness near the nucleus of its host galaxy, VV 306c. Pre-discovery upper limits constrain the time of explosion to within 200 d prior to discovery. While SN 2014ab declined by ∼1 mag over the course of our observations, the observed spectrum remained remarkably unchanged. Spectra exhibit an asymmetric emission-line profile with a consistently stronger blueshifted component, suggesting the presence of dust or a lack of symmetry between the far side and near side of the SN. The Pa β emission line shows a profile very similar to that of H α, implying that this stronger blueshifted component is caused either through obscuration by large dust grains, occultation by optically thick material, or a lack of symmetry between the far side and near side of the interaction region. Despite these asymmetric line profiles, our spectropolarimetric data show that SN 2014ab has little detected polarization after accounting for the interstellar polarization. We are likely seeing emission from a photosphere that has only small deviation from circular symmetry in the plane normal to our line of sight, but with either large-grain dust or significant asymmetry in the density of circumstellar material or SN ejecta along our line of sight. We suggest that SN 2014ab and SN 2010jl (as well as other SNe IIn) may be events with similar geometry viewed from different directions.