Submillimeter Emission from Water in the W3 Region

We have mapped the submillimeter emission from the 1(10)-1(01) transition of ortho-water in the W3 star-forming region. A 5'x5' map of the W3 IRS4 and W3 IRS5 region reveals strong water lines at half the positions in the map. The relative strength of the Odin lines compared to previous observations by SWAS suggests that we are seeing water emission from an extended region. Across much of the map the lines are double-peaked, with an absorption feature at -39 km/s; however, some positions in the map show a single strong line at -43 km/s. We interpret the double-peaked lines as arising from optically thick, self-absorbed water emission near the W3 IRS5, while the narrower blue-shifted lines originate in emission near W3 IRS4. In this model, the unusual appearance of the spectral lines across the map results from a coincidental agreement in velocity between the emission near W3 IRS4 and the blue peak of the more complex lines near W3 IRS5. The strength of the water lines near W3 IRS4 suggests we may be seeing water emission enhanced in a photon-dominated region.Comment: Accepted to A&A Letters as part of the special Odin issue; 4 page

First detection of NH3 (1,0 - 0,0) from a low mass cloud core: On the low ammonia abundance of the rho Oph A core

Odin has successfully observed the molecular core rho Oph A in the 572.5 GHz rotational ground state line of ammonia, NH3 (J,K = 1,0 - 0,0). The interpretation of this result makes use of complementary molecular line data obtained from the ground (C17O and CH3OH) as part of the Odin preparatory work. Comparison of these observations with theoretical model calculations of line excitation and transfer yields a quite ordinary abundance of methanol, X(CH3OH) = 3e-9. Unless NH3 is not entirely segregated from C17O and CH3OH, ammonia is found to be significantly underabundant with respect to typical dense core values, viz. X(NH3) = 8e-10.Comment: 4 pages, 2 figures, 2 tables, to appear in Astron. Astrophys. Letter

Reversal of infall in SgrB2(M) revealed by Herschel/HIFI observations of HCN lines at THz frequencies

To investigate the accretion and feedback processes in massive star formation, we analyze the shapes of emission lines from hot molecular cores, whose asymmetries trace infall and expansion motions. The high-mass star forming region SgrB2(M) was observed with Herschel/HIFI (HEXOS key project) in various lines of HCN and its isotopologues, complemented by APEX data. The observations are compared to spherically symmetric, centrally heated models with density power-law gradient and different velocity fields (infall or infall+expansion), using the radiative transfer code RATRAN. The HCN line profiles are asymmetric, with the emission peak shifting from blue to red with increasing J and decreasing line opacity (HCN to H$^{13}$CN). This is most evident in the HCN 12--11 line at 1062 GHz. These line shapes are reproduced by a model whose velocity field changes from infall in the outer part to expansion in the inner part. The qualitative reproduction of the HCN lines suggests that infall dominates in the colder, outer regions, but expansion dominates in the warmer, inner regions. We are thus witnessing the onset of feedback in massive star formation, starting to reverse the infall and finally disrupting the whole molecular cloud. To obtain our result, the THz lines uniquely covered by HIFI were critically important.Comment: A&A, HIFI special issue, accepte

Herschel observations of extra-ordinary sources: Detecting spiral arm clouds by CH absorption lines

We have observed CH absorption lines ($J=3/2, N=1 \leftarrow J=1/2, N=1$) against the continuum source Sgr~B2(M) using the \textit{Herschel}/HIFI instrument. With the high spectral resolution and wide velocity coverage provided by HIFI, 31 CH absorption features with different radial velocities and line widths are detected and identified. The narrower line width and lower column density clouds show `spiral arm' cloud characteristics, while the absorption component with the broadest line width and highest column density corresponds to the gas from the Sgr~B2 envelope. The observations show that each `spiral arm' harbors multiple velocity components, indicating that the clouds are not uniform and that they have internal structure. This line-of-sight through almost the entire Galaxy offers unique possibilities to study the basic chemistry of simple molecules in diffuse clouds, as a variety of different cloud classes are sampled simultaneously. We find that the linear relationship between CH and H$_2$ column densities found at lower $A_V$ by UV observations does not continue into the range of higher visual extinction. There, the curve flattens, which probably means that CH is depleted in the denser cores of these clouds.Comment: Accepted for publication in A&A, HIFI Special Issu

The use of virtual reality as a potential restorative environment in school during recess

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ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss and the recent star formation history of the inner disk and Bulge of the Galaxy. ISOGAL combines 7 and 15 micron ISOCAM observations - with a resolution of 6'' at worst - with DENIS IJKs data to determine the nature of the sources and theinterstellar extinction. We have observed about 16 square degrees with a sensitivity approaching 10-20mJy, detecting ~10^5 sources,mostly AGB stars,red giants and young stars. The main features of the ISOGAL survey and the observations are summarized in this paper,together with a brief discussion of data processing and quality. The primary ISOGAL products are described briefly (a full description is given in Schuller et al. 2003, astro-ph/0304309): viz. the images and theISOGAL-DENIS five-wavelength point source catalogue. The main scientific results already derived or in progress are summarized. These include astrometrically calibrated 7 and 15um images,determining structures of resolved sources; identification and properties of interstellar dark clouds; quantification of the infrared extinction law and source dereddening; analysis of red giant and (especially) AGB stellar populations in the central Bulge,determining luminosity,presence of circumstellar dust and mass--loss rate,and source classification,supplemented in some cases by ISO/CVF spectroscopy; detection of young stellar objects of diverse types,especially in the inner Bulge with information about the present and recent star formation rate; identification of foreground sources with mid-IR excess. These results are the subject of about 25 refereed papers published or in preparation.Comment: A&A in press. 19 pages,10 Ps figures; problems with figures fixe

First NH3 detection of the Orion Bar

Odin has successfully observed three regions in the Orion A cloud, i.e. Ori KL, Ori S and the Orion Bar, in the 572.5 GHz rotational ground state line of ammonia, ortho-NH3 (J,K) = (1,0) -> (0,0), and the result for the Orion Bar represents the first detection in an ammonia line. Several velocity components are present in the data. Specifically, the observed line profile from the Orion Bar can be decomposed into two components, which are in agreement with observations in high-J CO lines by Wilson et al. 2001. Using the source model for the Orion Bar by these authors, our Odin observation implies a total ammonia abundance of NH3/H2 = 5E-9.Comment: 4 pages with 2 figures, accepted for publication in A&

Impact of Vutrisiran on Quality of Life and Physical Function in Patients with Hereditary Transthyretin-Mediated Amyloidosis with Polyneuropathy

INTRODUCTION: Hereditary transthyretin (ATTRv; v for variant) amyloidosis, also known as hATTR amyloidosis, is a progressive and fatal disease associated with rapid deterioration of physical function and patients' quality of life (QOL). Vutrisiran, a subcutaneously administered RNA interference (RNAi) therapeutic that reduces hepatic production of transthyretin, was assessed in patients with ATTRv amyloidosis with polyneuropathy in the pivotal HELIOS-A study. METHODS: The phase 3 open-label HELIOS-A study investigated the efficacy and safety of vutrisiran in patients with ATTRv amyloidosis with polyneuropathy, compared with an external placebo group from the APOLLO study of the RNAi therapeutic patisiran. Measures of QOL and physical function were assessed. RESULTS: At month 18, vutrisiran improved Norfolk Quality of Life-Diabetic Neuropathy (Norfolk QOL-DN) total score (least squares mean difference [LSMD] in change from baseline [CFB]: –21.0; p = 1.84 × 10–10) and Norfolk QOL-DN domain scores, compared with external placebo. This benefit relative to external placebo was evident across all baseline polyneuropathy disability (PND) scores and most pronounced in patients with baseline PND scores I–II. Compared with external placebo, vutrisiran also demonstrated benefit in EuroQoL-Visual Analog Scale (EQ-VAS) score (LSMD in CFB: 13.7; nominal p = 2.21 × 10–7), 10-m walk test (LSMD in CFB: 0.239 m/s; p = 1.21 × 10–7), Rasch-built Overall Disability Score (LSMD in CFB: 8.4; p = 3.54 × 10–15), and modified body mass index (mBMI) (LSMD in CFB: 140.7; p = 4.16 × 10–15) at month 18. Overall, Norfolk QOL-DN, EQ-VAS, and mBMI improved from pretreatment baseline with vutrisiran, whereas all measures worsened from baseline in the external placebo group. At month 18, Karnofsky Performance Status was stable/improved from baseline in 58.2/13.1% with vutrisiran versus 34.7/8.1% with external placebo. CONCLUSION: Vutrisiran treatment provided significant clinical benefits in multiple measures of QOL and physical function in patients with ATTRv amyloidosis with polyneuropathy. Benefits were most pronounced in patients with earlier-stage disease, highlighting the importance of early diagnosis and treatment

Unknown cadaver: its historical and academic importance for human anatomy

Observações feitas na maioria das universidades brasileiras estrangeiras, e, inclusive, em algumas sobre o aspecto acadêmico do uso de cadáveres humanos como principal material que suporta e direciona a Anatomia Humana nos cursos da área da saúde, traz, dentre outras conclusões de caráter didático, uma questão de formação, muito mais importante do que uma simples questão de, apenas, informação universitária. Há de se concordar que, mesmo com o fabuloso avanço tecnológico e suas possibilidades, nossas universidades hoje, primam mais pela questão informativa do que propriamente pela formativa, ao passo que ternos consciência de que o ser humano necessita igualmente de ambas. Em consequência disto, o principal objetivo deste trabalho é enfocar o valor acadêmico do cadáver, evidenciando sua importante relação histórica, sem a qual a Anatomia não existiria e, certamente, a Medicina também não teria ultrapassado suas fronteiras limitadas do passado. O fato de ser este um trabalho realizado em uma universidade brasileira é revestido de responsabilidade e determinação em tentar colocar a figura do cadáver humano no lugar, no qual ele realmente deva estar, não apenas como simples material e instrumento de ensino da anatomia, mas também como lição de vida através da morte, criando Ciência e Arte, valorizando sua importância no contexto artístico e religioso, fatores estes imprescindíveis para a formação sócio-cultural humana. Por outro lado, este estudo com abordagem de caráter acadêmico, tornou-se dificil quanto a bibliografia específica, tendo sido feita portanto, quase toda a sua pesquisa em tratados históricos e anatômicos e, apenas alguns poucos trabalhos sobre a importância do cadáver para a Anatomia. Neste trabalho, procuramos usar ilustrações e figuras como documentação de caráter informativo e estético. Assim sendo, para uma abordagem mais ampla, o cadáver foi discutido desde sua relação histórica e acadêmica, até os dias de hoje, onde ainda se enfrenta, quase, as mesmas dificuldades do passado, no que diz respeito as questões de doação de corpo e órgãos, que deixaram de ser apenas institucionalmente acadêmicas, para ser mais rigorosamente sociais, segundo as Leis vigentes.Observations about most of brazilian universities and, even some of foreign ones, concerning the academic aspects of the use of human cadavers or corpses as the principal human anatomy method of studying, which maintain the basic courses of Health Sciences Field, that is, the cadaver or corpse himself should be also seen as a noble and magnificent way of transmitting knowledge and human values. Indeed, these observations have been showing some didactic results concerning much more, a matter of individual information than individual formation itself. Nowadays, this happens because scholasticism, differently from the past, seems to emphasize quantitative rather than qualitative teaching philosophy. We must admit that, even living in a technological era and being able to take advantages of its possibilities, our universities today emphasize much more the information itself than individual formation of our professionals of tomorrow, while we know that the individual needs both, equally. Therefore, the main goal of this work is focusing the academic importance of the human cadaver or corpse as a practical studying material, which is related to the own history of the practical Anatomy and consequently Medicine and, if it were not because of that, Medicine itself would not have gone beyond its limited frontiers of the past. On the other hand, the inedited academic meaning of this work became too difficult to come abroad, because of its specific bibliographical lack among scientific publications and, that's why, most of its text was found in the old Health Sciences, books and texts in general. However, another particular characteristic of this work is the great number of pictures and illustrations, which enrich the present text and substitute the lack of similar works' bibliography, In this work, the corpse is seen, from his historical relation and academical aspects the to present circumstances, where the need for anatomical study faces the same difficulties of the past, when Vesalius opened the way to the study of Human Anatomy, but as we know many years passed before Anatomy could be taught to medical students by means of dissection, the only method by which physicians and surgeons can fully acquire this knowledge. The scarcity of anatomical material seemed to be over at the present time, when laws were just enacted, such as specified law for the use of the corpse, organs and structures donation, that unfortunately did not solve the old and permanent problem, such as the absence of corpses for anatomical dissections.BV UNIFESP: Teses e dissertaçõe

Planck early results XX : New light on anomalous microwave emission from spinning dust grains

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