131 research outputs found

    Choriocarcinoma coexisting with epithelioid trophoblastic tumor of the uterine horn

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    • We report a choriocarcinoma coexisting with an epithelioid trophoblastic tumor. • Chemotherapy with methotrexate, etoposide, and actinomycin-D was efficacious. • Choriocarcinoma with epithelioid trophoblastic tumor may benefit from chemotherapy

    High abundance ratio of 13^{13}CO to C18^{18}O toward photon-dominated regions in the Orion-A giant molecular cloud

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    Aims. We derive physical properties such as the optical depths and the column densities of 13^{13}CO and C18^{18}O to investigate the relationship between the far ultraviolet (FUV) radiation and the abundance ratios between 13^{13}CO and C18^{18}O. Method. We have carried out wide-field (0.4 deg2^2) observations with an angular resolution of 25.8 arcsec (∼\sim 0.05 pc) in 13^{13}CO (JJ=1--0) and C18^{18}O (JJ=1--0) toward the Orion-A giant molecular cloud using the Nobeyama 45 m telescope in the on-the-fly mode. Results. Overall distributions and velocity structures of the 13^{13}CO and C18^{18}O emissions are similar to those of the 12^{12}CO (JJ=1--0) emission. The optical depths of the 13^{13}CO and C18O emission lines are estimated to be 0.05 << τ13CO\tau_{\rm ^{13}CO} << 1.54 and 0.01 << τC18O\tau_{\rm C^{18}O} << 0.18, respectively. The column densities of the 13^{13}CO and C18^{18}O emission lines are estimated to be 0.2 ×\times 1016^{16} << N13CON_{\rm ^{13}CO} << 3.7 ×\times 1017^{17} cm−2^{-2} and 0.4 ×\times 1015^{15} << NC18ON_{\rm C^{18}O} << 3.5 ×\times 1016^{16} cm−2^{-2}, respectively. The abundance ratios between 13^{13}CO and C18^{18}O, X13COX_{\rm ^{13}CO}/XC18OX_{\rm C^{18}O}, are found to be 5.7 - 33.0. The mean value of X13COX_{\rm ^{13}CO}/XC18OX_{\rm C^{18}O} in the nearly edge-on photon-dominated regions is found to be 16.47 ±\pm 0.10, which is a third larger than that the solar system value of 5.5. The mean value of X13COX_{\rm ^{13}CO}/XC18OX_{\rm C^{18}O} in the other regions is found to be 12.29 ±\pm 0.02. The difference of the abundance ratio is most likely due to the selective FUV photodissociation of C18^{18}O.Comment: 11 pages, 9 figures, Accepted to A&
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