14 research outputs found
SN 2019ehk: A Double-peaked Ca-rich Transient with Luminous X-Ray Emission and Shock-ionized Spectral Features
We present panchromatic observations and modeling of the Calcium-rich supernova (SN) 2019ehk in the star-forming galaxy M100 (d â 16.2 Mpc) starting 10 hr after explosion and continuing for ~300 days. SN 2019ehk shows a double-peaked optical light curve peaking at t = 3 and 15 days. The first peak is coincident with luminous, rapidly decaying Swift-XRTâdiscovered X-ray emission (L_x â 10âŽÂč erg sâ»Âč at 3 days; L_x â tâ»Âł), and a Shane/Kast spectral detection of narrow Hα and He II emission lines (v â 500 km sâ»Âč) originating from pre-existent circumstellar material (CSM). We attribute this phenomenology to radiation from shock interaction with extended, dense material surrounding the progenitor star at r (0.1â1) Ă 10Âčâ· cm. The photometric and spectroscopic properties during the second light-curve peak are consistent with those of Ca-rich transients (rise-time of t_r = 13.4 ± 0.210 days and a peak B-band magnitude of M_B = â15.1 ± 0.200 mag). We find that SN 2019ehk synthesized (3.1 ± 0.11) Ă 10â»ÂČ M_â of â”â¶Ni and ejected M_(ej) = (0.72 ± 0.040) Mâ total with a kinetic energy E_k = (1.8 ± 0.10) Ă 10â”â° erg. Finally, deep HST pre-explosion imaging at the SN site constrains the parameter space of viable stellar progenitors to massive stars in the lowest mass bin (~10 M_â) in binaries that lost most of their He envelope or white dwarfs (WDs). The explosion and environment properties of SN 2019ehk further restrict the potential WD progenitor systems to low-mass hybrid HeCO WD+CO WD binaries
Integral Medicine: Treating the WholeâPatient, Provider, Healthcare System
Purpose: Integral Medicine is an approach to health, disease and healing that invites multiple perspectives and modes of inquiry to synergistically support healing for patients, providers and health care systems.Approach: Integral Theory is a framework for organizing information that considers four perspectives essential to view the whole patient simultaneously â any or all of which may illuminate health or illness in a patient, population or system: âInterior-Individualâ (mind, psycho-spiritual development, etc.), âExterior-Individualâ (molecules, cells, organs, bodies, etc.), âInterior-Collectiveâ (cultural, ethical practices or norms, etc.), and âExterior-Collectiveâ (socioeconomic, environmental system, etc.).Major Points: In practice, the application of Integral Theory to patient care can lead to four quadrant diagnosis and therapy for everything from status asthmaticus to chronic fatigue syndrome. When applied to the personal and professional development of providers an Integral Theory framework may improve critical thinking, ethical reasoning, mindfulness and empathy. At the healthcare system design level, patients have better outcomes when cared for by organizations ranked as having better work environments (where nurses report low rates of burnout, adequate time with patients, good relationships with colleagues, and opportunities for advanced training and continuing education).Conclusions: Treating the whole person becomes more than simply including body, mind and spirit. The whole person includes multiple epistemological ways of knowing. Building on Integrative, Alternative, Complementary, Evidence-based Medicine, and Values-based care, Integral Medicine offers a methodology for integrating the âbestâ of each of these medical methodologies. Integral Theory, in this respect, can act as a meta-theory weaving together many of the converging concepts emerging in the service of whole patient care. Integral methodology also provides a common map/language for knowledge integration/translation and a shared inter-professional approach to whole patient care at the patient, population and health system levels
SN 2019ehk: A Double-peaked Ca-rich Transient with Luminous X-Ray Emission and Shock-ionized Spectral Features
We present panchromatic observations and modeling of the Calcium-rich
supernova 2019ehk in the star-forming galaxy M100 (d16.2 Mpc) starting
10 hours after explosion and continuing for ~300 days. SN 2019ehk shows a
double-peaked optical light curve peaking at and days. The first
peak is coincident with luminous, rapidly decaying -XRT
discovered X-ray emission ( at 3 days; ), and a Shane/Kast spectral detection of narrow H and
He II emission lines ( km/s) originating from pre-existent
circumstellar material. We attribute this phenomenology to radiation from shock
interaction with extended, dense material surrounding the progenitor star at
cm and the resulting cooling emission. We calculate a total CSM
mass of with particle density
. Radio observations indicate a significantly
lower density at larger radii. The photometric and
spectroscopic properties during the second light curve peak are consistent with
those of Ca-rich transients (rise-time of days and a peak
B-band magnitude of mag). We find that SN 2019ehk
synthesized of
and ejected
total with a kinetic energy .
Finally, deep pre-explosion imaging at the SN site constrains
the parameter space of viable stellar progenitors to massive stars in the
lowest mass bin (~10 ) in binaries that lost most of their He
envelope or white dwarfs. The explosion and environment properties of SN
2019ehk further restrict the potential WD progenitor systems to low-mass hybrid
HeCO WD + CO WD binaries.Comment: 51 pages, 27 figures. Accepted for publication in Ap