Observational and Physical Classification of Supernovae

This chapter describes the current classification scheme of supernovae (SNe). This scheme has evolved over many decades and now includes numerous SN Types and sub-types. Many of these are universally recognized, while there are controversies regarding the definitions, membership and even the names of some sub-classes; we will try to review here the commonly-used nomenclature, noting the main variants when possible. SN Types are defined according to observational properties; mostly visible-light spectra near maximum light, as well as according to their photometric properties. However, a long-term goal of SN classification is to associate observationally-defined classes with specific physical explosive phenomena. We show here that this aspiration is now finally coming to fruition, and we establish the SN classification scheme upon direct observational evidence connecting SN groups with specific progenitor stars. Observationally, the broad class of Type II SNe contains objects showing strong spectroscopic signatures of hydrogen, while objects lacking such signatures are of Type I, which is further divided to numerous subclasses. Recently a class of super-luminous SNe (SLSNe, typically 10 times more luminous than standard events) has been identified, and it is discussed. We end this chapter by briefly describing a proposed alternative classification scheme that is inspired by the stellar classification system. This system presents our emerging physical understanding of SN explosions, while clearly separating robust observational properties from physical inferences that can be debated. This new system is quantitative, and naturally deals with events distributed along a continuum, rather than being strictly divided into discrete classes. Thus, it may be more suitable to the coming era where SN numbers will quickly expand from a few thousands to millions of events.Comment: Extended final draft of a chapter in the "SN Handbook". Comments most welcom

How Distinctive are ADHD and RD? Results of a Double Dissociation Study

The nature of the comorbidity between Attention-Deficit/Hyperactivity Disorder (ADHD) and Reading Disability (RD) was examined using a double dissociation design. Children were between 8 and 12 years of age and entered into four groups: ADHD only (n = 24), ADHD+RD (n = 29), RD only (n = 41) and normal controls (n = 26). In total, 120 children participated in the study; 38 girls and 82 boys. Both ADHD and RD were associated with impairments in inhibition and lexical decision, although inhibition and lexical decision were more severely impaired in RD than in ADHD. Visuospatial working memory deficits were specific to children with only ADHD. It is concluded that there was overlap on lexical decision and to a lesser extent on inhibition between ADHD and RD. In ADHD, impairments were dependent on IQ, which suggest that the overlap in lexical decision and inhibition is different in origin for ADHD and RD. The ADHD only group was specifically characterized by deficits in visuospatial working memory. Hence, no double dissociation between ADHD and RD was found on executive functioning and lexical decision

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Transtornos depressivos em crianças com leucemia linfoide aguda e com insuficiência renal crônica terminal: estudo de série de casos Depressive disease in children with acute lymphocytic leukemia and end stage of renal disease: case series study

OBJETIVO: Investigar a presença de transtornos depressivos em crianças portadoras de leucemia linfoide aguda (LLA) e insuficiência renal crônica terminal (IRCT) atendidas no IMIP. MÉTODO: Estudo descritivo do tipo série de casos, composto por 52 crianças entre 8 e 15 anos portadoras de LLA e de IRCT. RESULTADOS: Três (5,8%) casos preenchiam os critérios para episódio depressivo maior (EDM), sendo dois portadores de IRCT e um portador de LLA. Oito (15,4%) preenchiam os critérios para transtorno distímico (TD), todos eles portadores de IRCT. A associação entre faixa etária e EDM não foi significativa (p=0,327). Entretanto, a faixa etária foi significante em relação ao TD (p=0,014), todos os seus portadores tinham entre 12 e 15 anos de idade. A associação entre os transtornos depressivos e o tempo de evolução da doença de base não foi significante. Contudo, observou-se uma tendência a quanto maior o tempo de evolução da doença de base, maior a associação com o TD. CONCLUSÃO: A frequência de EDM ficou dentro da faixa encontrada na literatura para escolares saudáveis, entretanto, a de TD foi mais alta. Não foram encontradas diferenças significantes entre as faixas etárias no diagnóstico de EDM. Porém, corroborando a literatura, a faixa etária maior prevaleceu em relação ao TD.<br>OBJECTIVE: To Investigate the presence of depressive disease in children with acute lymphocytic leukemia (ALL) and end stage of renal disease (ESRD). METHOD: A case series study including 52 children suffering of ALL or ESRD aged 8 to 15 years. RESULTS: Three patients (5.8%) had major depressive episode (MDE), two of them with ESRD and one with ALL. Eight patients (15.4%) had dysthymic disorder (DD), all of them had ESRD. The association between age and MDE was not meaningful. On other hand, the association between age and DD was significant, and all of the patients aged between 12 and 15 years. The association between depressive diseases and evolution time of base disease was not significant. However, it was observed that the bigger the time of base disease evolution, the bigger the association with DD. CONCLUSION: The frequency of MED was not different from the literature, but the frequency of DD was higher. In opposition to what was expected, there wasn't difference between the ages in MED. However, in agreement with the literature, it prevailed the highest ages in DD