Awakenings: An Equine Assisted Learning Research Project

Objective. The purpose of this pilot study was to determine if and how the Awakenings Equine Assisted Learning program was effective at improving the professionalism, confidence, communication skills and adaptability of students preparing for careers as Anesthesiologist Assistants. Background. Equine Assisted Learning (EAL) is a rapidly growing experiential model that utilizes horses to enhance participants\u27 awareness of their own non-verbal language, communication styles, projection of self-confidence and competence, and problem-solving abilities (Chandler, 2012; Green, 2012, 2013; Kane, 2012; Trotter, 2012). Methods. As a part of their regular educational and clinical rotations, first year students in the Anesthesiologist Assistant (AA) program participated in a 6- week training that included weekly, 2 -hour Equine Assisted Learning (EAL) sessions. Each session, the AA students participated in a 2- hour experiential equine assisted activity, specifically designed to address a certain target area necessary for their development as professionals in this field. The participants completed a pre and post assessment with 93 items that measured development as they relate to the EAL sessions. Results. The data was analyzed using t-tests, exploratory factor analysis, and qualitative self-reports. Confidence, empathy, awareness, and communication were the most significant factors. Conclusion. The qualitative data reinforced the quantitative findings that showed significant improvement in the objective factors as a result of the EAL sessions

OVI, NV and CIV in the Galactic Halo: II. Velocity-Resolved Observations with Hubble and FUSE

We present a survey of NV and OVI (and where available CIV) in the Galactic halo, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE) and the Hubble Space Telescope (HST) along 34 sightlines. These ions are usually produced in nonequilibrium processes such as shocks, evaporative interfaces, or rapidly cooling gas, and thus trace the dynamics of the interstellar medium. Searching for global trends in integrated and velocity-resolved column density ratios, we find large variations in most measures, with some evidence for a systematic trend of higher ionization (lower NV/OVI column density ratio) at larger positive line-of-sight velocities. The slopes of log[N(NV)/N(OVI)] per unit velocity range from -0.015 to +0.005, with a mean of -0.0032+/-0.0022(r)+/-0.0014(sys) dex/(km/s). We compare this dataset with models of velocity-resolved high-ion signatures of several common physical structures. The dispersion of the ratios, OVI/NV/CIV, supports the growing belief that no single model can account for hot halo gas, and in fact some models predict much stronger trends than are observed. It is important to understand the signatures of different physical structures to interpret specific lines of sight and future global surveys.Comment: ApJ in press 43 pages, 22 fig

Discovery of an Unbound Hyper-Velocity Star in the Milky Way Halo

We have discovered a star, SDSS J090745.0+024507, leaving the Galaxy with a heliocentric radial velocity of +853+-12 km/s, the largest velocity ever observed in the Milky Way halo. The star is either a hot blue horizontal branch star or a B9 main sequence star with a heliocentric distance ~55 kpc. Corrected for the solar reflex motion and to the local standard of rest, the Galactic rest-frame velocity is +709 km/s. Because its radial velocity vector points 173.8 deg from the Galactic center, we suggest that this star is the first example of a hyper-velocity star ejected from the Galactic center as predicted by Hills and later discussed by Yu & Tremaine. The star has [Fe/H]~0, consistent with a Galactic center origin, and a travel time of <80 Myr from the Galactic center, consistent with its stellar lifetime. If the star is indeed traveling from the Galactic center, it should have a proper motion of 0.3 mas/yr observable with GAIA. Identifying additional hyper-velocity stars throughout the halo will constrain the production rate history of hyper-velocity stars at the Galactic center.Comment: 4 pages, submitted to ApJ Letter

Metal Abundances in the Magellanic Stream

We report on the first metallicity determination for gas in the Magellanic Stream, using archival HST GHRS data for the background targets Fairall 9, III Zw 2, and NGC 7469. For Fairall 9, using two subsequent HST revisits and new Parkes Multibeam Narrowband observations, we have unequivocally detected the MSI HI component of the Stream (near its head) in SII1250,1253 yielding a metallicity of [SII/H]=-0.55+/-0.06(r)+/-0.2(s), consistent with either an SMC or LMC origin and with the earlier upper limit set by Lu et al. (1994). We also detect the saturated SiII1260 line, but set only a lower limit of [SiII/H]>-1.5. We present serendipitous detections of the Stream, seen in MgII2796,2803 absorption with column densities of (0.5-1)x10^13 cm^-2 toward the Seyfert galaxies III Zw 2 and NGC 7469. These latter sightlines probe gas near the tip of the Stream (80 deg down-Stream of Fairall 9). For III Zw 2, the lack of an accurate HI column density and the uncertain MgIII ionization correction limits the degree to which we can constrain [Mg/H]; a lower limit of [MgII/HI]>-1.3 was found. For NGC 7469, an accurate HI column density determination exists, but the extant FOS spectrum limits the quality of the MgII column density determination, and we conclude that [MgII/HI]>-1.5. Ionization corrections associated with MgIII and HII suggest that the corresponding [Mg/H] may range lower by 0.3-1.0 dex. However, an upward revision of 0.5-1.0 dex would be expected under the assumption that the Stream exhibits a dust depletion pattern similar to that seen in the Magellanic Clouds. Remaining uncertainties do not allow us to differentiate between an LMC versus SMC origin to the Stream gas.Comment: 30 pages, 8 figures, LaTeX (aaspp4), also available at http://casa.colorado.edu/~bgibson/publications.html, accepted for publication in The Astronomical Journa

Chemical abundance patterns in the inner Galaxy: the Scutum Red Supergiant Clusters

The location of the Scutum Red-Supergiant (RSG) clusters at the end of the Galactic Bar makes them an excellent probe of the Galaxy's secular evolution; while the clusters themselves are ideal testbeds in which to study the predictions of stellar evolutionary theory. To this end, we present a study of the RSGs' surface abundances using a combination of high-resolution H-band spectroscopy and spectral synthesis analysis. We provide abundance measurements for elements C, O, Si, Mg, Ti, and Fe. We find that the surface abundances of the stars studied are consistent with CNO burning and deep, rotationally enhanced mixing. The average a/Fe ratios of the clusters are solar, consistent with a thin-disk population. However, we find significantly sub-solar Fe/H ratios for each cluster, a result which strongly contradicts a simple extrapolation of the Galactic metallicity gradient to lower Galacto-centric distances. We suggest that a simple one-dimensional parameterization of the Galaxy's abundance patterns is insufficient at low Galactocentric distances, as large azimuthal variations may be present. Indeed, we show that the abundances of O, Si and Mg are consistent with independent measurements of objects in similar locations in the Galaxy. In combining our results with other data in the literature, we present evidence for large-scale (~kpc) azimuthal variations in abundances at Galacto-centric distances of 3-5kpc. While we cannot rule-out that this observed behaviour is due to systematic offsets between different measurement techniques, we do find evidence for similar behaviour in a study of the barred-spiral galaxy NGC4736 which uses homogeneous methodology. We suggest that these azimuthal abundance variations could result from the intense but patchy star formation driven by the potential of the central bar.Comment: 13 pages, 9 figures, accepted to Ap

Shedding Light on Vampires: The Phylogeny of Vampyrellid Amoebae Revisited

With the advent of molecular phylogenetic techniques the polyphyly of naked filose amoebae has been proven. They are interspersed in several supergroups of eukaryotes and most of them already found their place within the tree of life. Although the ‘vampire amoebae’ have attracted interest since the middle of the 19th century, the phylogenetic position and even the monophyly of this traditional group are still uncertain. In this study clonal co-cultures of eight algivorous vampyrellid amoebae and the respective food algae were established. Culture material was characterized morphologically and a molecular phylogeny was inferred using SSU rDNA sequence comparisons. We found that the limnetic, algivorous vampyrellid amoebae investigated in this study belong to a major clade within the Endomyxa Cavalier-Smith, 2002 (Cercozoa), grouping together with a few soil-dwelling taxa. They split into two robust clades, one containing species of the genus Vampyrella Cienkowski, 1865, the other containing the genus Leptophrys Hertwig & Lesser, 1874, together with terrestrial members. Supported by morphological data these clades are designated as the two families Vampyrellidae Zopf, 1885, and Leptophryidae fam. nov. Furthermore the order Vampyrellida West, 1901 was revised and now corresponds to the major vampyrellid clade within the Endomyxa, comprising the Vampyrellidae and Leptophryidae as well as several environmental sequences. In the light of the presented phylogenetic analyses morphological and ecological aspects, the feeding strategy and nutritional specialization within the vampyrellid amoebae are discussed

Equine-Assisted Psychotherapy with Couples and Families: A Relational Approach

Written by internationally renowned equine-assisted mental health professionals, this edited collection teaches counselors how to design and implement equine-assisted mental health interventions for different populations and various challenges. Supported by ethical considerations and theoretical framework, chapters cover common issues including depression, anxiety, grief, ADHD, autism, eating disorders, substance abuse, self-esteem, social skills and communication, couples and family work, and professional development. Each chapter provides practical tips for implementing treatment strategies, case studies with transcript analyses, and sample session notes. This book will appeal to both the expert equine-assisted mental health counselor and the seasoned counselor who is open to partnering with an equine practitioner to help their clients in new and innovative ways.https://nsuworks.nova.edu/shss_facbooks/1103/thumbnail.jp

Awakenings: An Equine Assisted Learning Research Project

Objective. The purpose of this pilot study was to determine if and how the Awakenings Equine Assisted Learning program was effective at improving the professionalism, confidence, communication skills and adaptability of students preparing for careers as Anesthesiologist Assistants. Background. Equine Assisted Learning (EAL) is a rapidly growing experiential model that utilizes horses to enhance participants\u27 awareness of their own non­verbal language, communication styles, projection of self-confidence and competence, and problem-solving abilities (Chandler, 2012; Green, 2012, 2013; Kane, 2012; Trotter, 2012). Methods. As a part of their regular educational and clinical rotations, first year students in the Anesthesiologist Assistant (AA) program participated in a 6­ week training that included weekly, 2 ­hour Equine Assisted Learning (EAL) sessions. Each session, the AA students participated in a 2­ hour experiential equine assisted activity, specifically designed to address a certain target area necessary for their development as professionals in this field. The participants completed a pre and post assessment with 93 items that measured development as they relate to the EAL sessions. Results. The data was analyzed using t-tests, exploratory factor analysis, and qualitative self-reports. Confidence, empathy, awareness, and communication were the most significant factors. Conclusion. The qualitative data reinforced the quantitative findings that showed significant improvement in the objective factors as a result of the EAL sessions

Triggering Transformations: An Equine Assisted Approach to the Treatment of Substance Abuse

This chapter describes a relational, solution-focused approach to Equine-assisted psychotherapy (EAP) that incorporates attention to mindfulness, allowing clients struggling with substance abuse to work on their individual goals alongside other group participants. In the treatment of substance abuse, mindfulness practices may help clients avoid relapse by increasing their awareness of negative patterns of thoughts and emotions that could increase the likelihood of relapse triggers. Clinically, the combination of the equine-assisted experiential model and a solution-focused emphasis offers opportunities for heightened awareness and transformation. EAP approaches have been applied to many different clinical concerns, including substance abuse, eating disorders, domestic violence, trauma, post-traumatic stress disorder, and physical or sexual abuse. The horses assist the therapists in shining light on the clients\u27 abilities and strengths in relation to their problem. Clinical approaches that address the addiction without considering the clients\u27 strengths, resources, and resilience miss critical opportunities to engage clients in a collaborative process that can anchor their decision to remain sober.https://nsuworks.nova.edu/shss_facbooks/1127/thumbnail.jp

Examining Equine Facilitated Psychotherapy as a Complement to Standard Care for Foster Youth in Residential Treatment

The project represents a university-community partnership among FIU-BRIDGE, Nova Southeastern University’s (NSU) Family Therapy Program, Stable Place, a non‐profit in its fifth year of providing equine facilitated psychotherapy in the community, and the SOS Children’s Village, a foster child residential treatment facility. This project is offering Equine Facilitated Psychotherapy as an adjunctive treatment for South Florida foster youth in a residential treatment program. We will examine the impact of participation on the participant’s quality of life including self‐confidence, self-efficacy, mindfulness and interpersonal relations, as well as anxiety and depressive symptoms. The specific clinical training model proposed will provide a consistent, theoretically based approach to EFP (Green, in press, 2014, 2013, 2011). The EFP clinical model utilizes a number of Equine Assisted Growth and Learning Association (EAGALA)‐based and other standard equine facilitated activities (Faa‐Thompson, 2012; Trotter, 2012); however, the clinical processing of those activities is consistently informed by systemic, brief therapy traditions (Cade & O’Hanlon, 1993; Hoyt, 1996) and was developed by Dr. Green at NSU