{"paper":{"title":"Mapping Jet-ISM Interactions in X-ray Binaries with ALMA: A GRS 1915$+$105 Case Study","arxiv_id":"1712.00432","primary_cat":"astro-ph.HE","submitted_at":"2017-12-01T18:08:08+00:00","version_compiled":"v1"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. No sentence in this record was written by a language model.","schema":"pith.compiled-record/v0","status":"compiled","abstract":{"source":"arXiv listing abstract v1","sentences":[{"i":0,"p":1.0,"id":"s0","own":true,"role":"contribution","text":"We present Atacama Large Millimetre/Sub-Millimetre Array (ALMA) observations of IRAS 19132+1035, a candidate jet-ISM interaction zone near the black hole X-ray binary (BHXB) GRS 1915+105.","hedge":{"p":0.56,"label":"asserted"},"own_p":0.93,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.26,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":1.0,"interpretation":0.0}},{"i":1,"p":0.95,"id":"s1","own":true,"role":"method","text":"With these ALMA observations (combining data from the 12 m array and the Atacama Compact Array), we map the molecular line emission across the IRAS 19132+1035 region.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.96,"main_claim_p":0.02,"quantitative":false,"quantitative_p":0.14,"role_probabilities":{"gap":0.0,"method":0.95,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.05,"interpretation":0.0}},{"i":2,"p":0.94,"id":"s2","own":true,"role":"result","text":"We detect emission from the $^{12}$CO [$J=2-1$], $^{13}$CO [$\\nu=0$, $J=2-1$], C$^{18}$O [$J=2-1$], ${\\rm H}_{2}{\\rm CO}$ [$J=3_{0,3}-2_{0,2}$], ${\\rm H}_{2}{\\rm CO}$ [$J=3_{2,2}-2_{2,1}$], ${\\rm H}_{2}{\\rm CO}$ [$J=3_{2,1}-2_{2,0}$], SiO [$\\nu=0$, $J=5-4$], CH$_3$OH [$J=4_{2,2}-3_{1,2}$], and CS [$\\nu=0$, $J=5-4$] transitions.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.97,"main_claim_p":0.02,"quantitative":true,"quantitative_p":0.63,"role_probabilities":{"gap":0.0,"method":0.04,"result":0.94,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.02,"interpretation":0.0}},{"i":3,"p":0.85,"id":"s3","own":true,"role":"interpretation","text":"Given the morphological, spectral, and kinematic properties of this molecular emission, we present several lines of evidence that support the presence of a jet-ISM interaction at this site, including a jet-blown cavity in the molecular gas.","hedge":{"p":0.56,"label":"hedged_possibility"},"own_p":0.93,"main_claim_p":0.32,"quantitative":false,"quantitative_p":0.05,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.15,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.0,"interpretation":0.85}},{"i":4,"p":0.77,"id":"s4","own":true,"role":"interpretation","text":"This compelling new evidence identifies this site as a jet-ISM interaction zone, making GRS 1915$+$105 the third Galactic BHXB with at least one conclusive jet-ISM interaction zone.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.86,"main_claim_p":0.66,"quantitative":true,"quantitative_p":0.91,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.21,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.02,"interpretation":0.77}},{"i":5,"p":0.6,"id":"s5","own":true,"role":"result","text":"However, we find that this interaction occurs on much smaller scales than was postulated by previous work, where the BHXB jet does not appear to be dominantly powering the entire IRAS 19132+1035 region.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.96,"main_claim_p":0.11,"quantitative":true,"quantitative_p":0.88,"role_probabilities":{"gap":0.0,"method":0.0,"result":0.6,"background":0.0,"limitation":0.06,"future_work":0.0,"contribution":0.0,"interpretation":0.34}},{"i":6,"p":0.98,"id":"s6","own":true,"role":"result","text":"Using estimates of the ISM conditions in the region, we utilize the detected cavity as a calorimeter to estimate the time-averaged power carried in the GRS 1915+105 jets of $(8.4^{+7.7}_{-8.1})\\times10^{32}\\,{\\rm erg\\,s}^{-1}$.","hedge":{"p":0.99,"label":"asserted"},"own_p":0.97,"main_claim_p":0.07,"quantitative":true,"quantitative_p":0.99,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.98,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.01,"interpretation":0.0}},{"i":7,"p":0.93,"id":"s7","own":true,"role":"interpretation","text":"Overall, our analysis demonstrates that molecular lines are excellent diagnostic tools to identify and probe jet-ISM interaction zones near Galactic 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