Chemical and kinematical properties of BSSs and HB stars in NGC 6397

We used three sets of high-resolution spectra acquired with the multifiber facility FLAMES at the Very Large Telescope of the European Southern Observatory to investigate the chemical and kinematical properties of a sample of 42 horizontal branch (HB) stars, 18 Blue Straggler Stars (BSSs) and 86 main sequence turn-off and sub-giant branch stars in the nearby globular cluster NGC 6397. We measured rotational velocities and Fe, O and Mg abundances. All the unevolved stars in our sample turn out to have low rotational velocites (v sin i< 10\kms), while HB stars and BSSs show a broad distribution, with values ranging from 0 to 70 \kms. For HB stars with T<10500 K there is a clear temperature-oxygen anti-correlation, that can be understood if the star position along the HB is mainly determined by the He content. The hottest BSSs and HB stars (with temperatures T>8200 K and T> 10500 K, respectively) also show significant deviations in their iron abundance with respect to the cluster metallicity (as traced by the unevolved stars, [Fe/H]=-2.12). While similar chemical patterns have been already observed in other hot HB stars, this is the first evidence ever collected for BSSs. We interprete these abundance anomalies as due to the metal radiative levitation, occurring in stars with shallow or no convective envelopes

Disc instability in RS Ophiuchi: a path to Type Ia supernovae?

We study the stability of disc accretion in the recurrent nova RS Ophiuchi. We construct a one-dimensional time-dependent model of the binary-disc system, which includes viscous heating and radiative cooling and a self-consistent treatment of the binary potential. We find that the extended accretion disc in this system is always unstable to the thermal-viscous instability, and undergoes repeated disc outbursts on ~10-20yr time-scales. This is similar to the recurrence time-scale of observed outbursts in the RS Oph system, but we show that the disc's accretion luminosity during outburst is insufficient to explain the observed outbursts. We explore a range of models, and find that in most cases the accretion rate during outbursts reaches or exceeds the critical accretion rate for stable nuclear burning on the white dwarf surface. Consequently we suggest that a surface nuclear burning triggered by disc instability may be responsible for the observed outbursts. This allows the white dwarf mass to grow over time, and we suggest that disc instability in RS Oph and similar systems may represent a path to Type Ia supernovae.Comment: 8 pages, 5 figures. Accepted for publication in MNRA

Young star clusters in the Large Magellanic Cloud: NGC 1805 and NGC 1818

We present colour-magnitude diagrams for two rich (~10^4 Msun) Large Magellanic Cloud star clusters with ages ~10^7 years, constructed from optical and near-infrared data obtained with the Hubble Space Telescope. These data are part of an HST project to study LMC clusters with a range of ages. In this paper we investigate the massive star content of the young clusters, and determine the cluster ages and metallicities, paying particular attention to Be star and blue straggler populations and evidence of age spreads. We compare our data to detailed stellar population simulations to investigate the turn-off structure of ~25 Myr stellar systems, highlighting the complexity of the blue straggler phenomenon.Comment: 15 pages, accepted for publication in MNRAS, postscript version with higher quality figures available from http://www.ast.cam.ac.uk/~raj/biblio.htm

Mass segregation in young compact star clusters in the Large Magellanic Cloud: I. Data and Luminosity Functions

We have undertaken a detailed analysis of HST/WFPC2 and STIS imaging observations, and of supplementary wide-field ground-based observations obtained with the NTT of two young ~10-25 Myr) compact star clusters in the LMC, NGC 1805 and NGC 1818. The ultimate goal of our work is to improve our understanding of the degree of primordial mass segregation in star clusters. This is crucial for the interpretation of observational luminosity functions (LFs) in terms of the initial mass function (IMF), and for constraining the universality of the IMF. We present evidence for strong luminosity segregation in both clusters. The LF slopes steepen with cluster radius; in both NGC 1805 and NGC 1818 the LF slopes reach a stable level well beyond the clusters' core or half-light radii. In addition, the brightest cluster stars are strongly concentrated within the inner ~4 R_hl. The global cluster LF, although strongly nonlinear, is fairly well approximated by the core or half-light LF; the (annular) LFs at these radii are dominated by the segregated high-luminosity stars, however. We present tentative evidence for the presence of an excess number of bright stars surrounding NGC 1818, for which we argue that they are most likely massive stars that have been collisionally ejected from the cluster core. We therefore suggest that the cores of massive young stars clusters undergo significant dynamical evolution, even on time-scales as short as ~25 Myr.Comment: 19 pages, incl. 10 embedded postscript figures, MNRAS, resubmitted (referee's comments included

Massive stars in the giant molecular cloud G23.3−0.3 and W41

Context. Young massive stars and stellar clusters continuously form in the Galactic disk, generating new Hii regions within their natal giant molecular clouds and subsequently enriching the interstellar medium via their winds and supernovae.Aims. Massive stars are among the brightest infrared stars in such regions; their identification permits the characterisation of the star formation history of the associated cloud as well as constraining the location of stellar aggregates and hence their occurrence as a function of global environment.Methods. We present a stellar spectroscopic survey in the direction of the giant molecular cloud G23.3−0.3. This complex is located at a distance of ~4–5 kpc, and consists of several Hii regions and supernova remnants.Results. We discovered 11 OfK+ stars, one candidate luminous blue variable, several OB stars, and candidate red supergiants. Stars with K-band extinction from ~1.3–1.9 mag appear to be associated with the GMC G23.3−0.3; O and B-types satisfying this criterion have spectrophotometric distances consistent with that of the giant molecular cloud. Combining near-IR spectroscopic and photometric data allowed us to characterize the multiple sites of star formation within it. The O-type stars have masses from ~25–45 M⊙, and ages of 5–8 Myr. Two new red supergiants were detected with interstellar extinction typical of the cloud; along with the two RSGs within the cluster GLIMPSE9, they trace an older burst with an age of 20–30 Myr. Massive stars were also detected in the core of three supernova remnants – W41, G22.7−0.2, and G22.7583−0.4917.Conclusions. A large population of massive stars appears associated with the GMC G23.3−0.3, with the properties inferred for them indicative of an extended history of stars formation

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

What Patient And Psychologist Characteristics Are Important In Competency For Physician-Assisted Suicide Evaluations?

The practice of physician-assisted suicide (PAS) is currently legal in Oregon (Oregon Death With Dignity Act, 1995), Washington (Washington Death With Dignity Act, 2008), and Montana (Baxter v. Montana, 2009). In an effort to identify important characteristics of patients and clinicians involved in evaluations of competence to request PAS, 216 licensed psychologists from Oregon and Montana were surveyed regarding their attitudes toward PAS and their personal and professional experiences with suicide. They were also asked to make a competence decision for a patient requesting PAS based on a case vignette. Cognitive ability, as indicated by a question regarding the importance of cognitive ability and components of competence that rely on reasoning skills, was the only patient factor that significantly predicted competence decisions. Results also suggested that personal characteristics of clinicians, particularly whether someone in their personal life had ever attempted suicide and their willingness to support a family member\u27s choice of PAS, influence their decision regarding the competence of the patient. Exploratory analyses also revealed that clinicians consider perceived burdensomeness to be of little importance when conducting a competence evaluation for PAS. In all, the largest effects were observed for the experimental vignette condition, clinician personal experience with attempted suicide, and clinician perceived importance of patient MacArthur Competence Assessment Tool for Treatment- Appreciation scores. The implications of these results are discussed, centering on recommendations for clinicians considering participating in competence evaluations for PAS and future directions for research

Social Determinants Associated with Physical Activity among Indigenous Adults at the University of Saskatchewan

Colonization impacts Indigenous Peoples’ way of life, culture, language, community structure and social networks. Links between social determinants of health and physical activity (PA) among Indigenous Peoples in Saskatchewan, with 16% Indigenous residents, are unclear. This cross-sectional study guided by Indigenous Community Advisors, compared moderate-to-vigorous PA (MVPA), traditional Indigenous PA and musculoskeletal PA with social determinants of Indigenous, (n=124), including First Nations (n=80, including 57 Cree/Nehiyawak) and Mtis (n=41), adults in Saskatchewan. Participants completed Godin-Shephard Leisure-Time PA, Social Support Index and traditional Indigenous PA participation questionnaires. Regression associated positive perception of social support with MVPA (R=0.306, p=0.02), while residential school experiences (R=0.338, p=0.02) and community support (R=0.412, p=0.01) were associated with traditional Indigenous PA participation. Among Mtis, discrimination experiences were associated with traditional Indigenous PA participation (R=0.459, p=0.01). Traditional Indigenous PA participation was associated with community support among First Nations (R=0.263, p=0.04), and also foster care placement (R=0.480, p=0.01) for Cree/Nehiyawak First Nations specifically. Among Cree/Nehiyawak, family support (R=0.354, p=0.04), discrimination experiences (R=0.531, p=0.01) and positive perceptions of support (R=0.610, p=0.003) were associated with musculoskeletal PA. Greater community, family and perceived social support, and experiences of discrimination, residential school and foster care are associated with more PA for Indigenous Peoples. Novelty: • Positive support perceptions predict physical activity among Indigenous Peoples • Family support, discrimination experiences and positive support perceptions predict physical activity for Cree/Nehiyawak First Nations. Traditional physical activity was predicted by residential school experiences and community support (Indigenous Peoples), discrimination experiences (Mtis), community support (First Nations), and foster care experiences (Cree/Nehiyawak)The accepted manuscript in pdf format is listed with the files at the bottom of this page. The presentation of the authors' names and (or) special characters in the title of the manuscript may differ slightly between what is listed on this page and what is listed in the pdf file of the accepted manuscript; that in the pdf file of the accepted manuscript is what was submitted by the author