A new semi-automatic approach is employed to carry out the abundance analysis of highresolution spectra of HD 41076 and HD 148330 obtained recently with the spectropolarimetre ESPaDOnS at the CFHT. This approach allows to prepare in a semi-automatic mode the input data for the modified ZEEMAN2 code and to analyse several hundreds of line profiles in sequence during a single run. It also provides more information on abundance distribution for each chemical element at the deeper atmospheric layers. Our analysis of the Balmer profiles observed in the spectra of HD 41076 and HD 148330 has resulted in the estimates of their effective temperature, gravity, metallicity and radial velocity. The respective models of stellar atmosphere have been calculated with the code PHOENIX and used to carry out abundance analysis employing the modified ZEEMAN2 code. The analysis shows a deficit of the C, N, F, Mg, Ca, Ti, V, Cu, Y, Mo, Sm and Gd, and overabundance of Cr, Mn, Fe, Co, Ni, Sr, Zr, Ba, Ce, Nd and Dy in the stellar atmosphere of HD 41076. In the atmosphere of HD 148330, the C, N and Mo appear to be underabundant, while the Ne, Na, Al, Si, P, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Zn, Sr, Y, Zr, Ba, Ce, Pr, Nd, Sm, Eu, Gd and Dy are overabundant. We also have found signatures of vertical abundance stratification of Fe, Ti, Cr and Mn in HD 41076, and of Fe, Ti, V, Cr, Mn, Y, Zr, Ce, Nd, Sm and Gd in HD 148330.

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We present the first results of the estimation of gravity and effective temperature for some poorly studied chemically peculiar stars that were recently observed with the spectropolarimeter ESPaDOnS at CFHT. We have analyzed the spectra of HD71030, HD95608 and HD116235 to determine their radial velocity, Vsin(i) and the average abundance of several chemical species. We have also analyzed our results to verify for possible vertical abundance stratification of iron and chromium in these stars.Comment: 2 pages, 2 figures, IAU 302 "Magnetic fields throughout stellar evolution

This chapter articulates a theoretical model for a creative arts therapy group for trans and non-binary youth aged 14 to 18 years in Canada. With the inclusion of audio extracts, this chapter provides the reader with a glimpse into the realities of the group and it highlights lessons learned from the work achieved. From the point of view of a trans music therapist, this chapter covers recommendations for clinical work in this setting. This chapter also discusses the importance of an anti-oppressive approach to allow expression of complex emotions to arise and be shared. Considering artistic expression as a tool to convey openness, I discuss the needs of trans and non-binary youth for community, as a means to be supported and witnessed. Finally, the chapter touches on the work achieved outside the group that allowed for systemic change and parental, social, and legal support. This chapter aims to provide an operational overview of the ways in which queer and trans music therapy can be clinically realized.

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