{"total":12,"items":[{"citing_arxiv_id":"2606.26827","ref_index":159,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing outflow physics through CH$_3$CN and CH$_3$OH chemistry","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T10:06:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"The CH₃OH/CH₃CN ratio in the S68N outflow is constant at ~100-200 and matches gas-phase astrochemical models only when cosmic-ray ionization rates are raised to ~10^{-14} s^{-1}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25794","ref_index":114,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Substructures in Planet-Forming Disks with the SKAO","primary_cat":"astro-ph.EP","submitted_at":"2026-06-24T13:13:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"This review chapter discusses open questions on protoplanetary disk substructures and how SKA-Mid continuum observations at 12.5 GHz can help resolve them.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20265","ref_index":87,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"UCLCHEM 4.0: An open source gas-grain astrochemistry simulation framework","primary_cat":"astro-ph.GA","submitted_at":"2026-06-18T14:13:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"UCLCHEM 4.0 is an updated open-source framework that solves time-dependent gas-grain chemical networks with built-in parametrizations for cloud collapse, cores, and shocks.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.08607","ref_index":29,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"ALMA High-resolution Observation of the HH46/47 Outflow/disk/envelope System","primary_cat":"astro-ph.GA","submitted_at":"2026-06-07T12:40:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"New ALMA data at 50 au resolution of HH46/47 shows a rotating-infalling envelope to disk transition at 30 au around a 0.3 solar-mass protostar, with outflow shells expanding radially and supporting entrainment over disk-wind origin.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.07388","ref_index":13,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"ALMAGAL IX. The chemical complexity of AG318.9477-00.1960: A line-identification template for ALMAGAL","primary_cat":"astro-ph.GA","submitted_at":"2026-06-05T15:26:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LTE analysis of ALMA data for AG318-c9 yields molecular parameters and spatial maps for three COMs, compared to G31 as a line-identification template for the ALMAGAL survey.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03261","ref_index":150,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43","primary_cat":"astro-ph.GA","submitted_at":"2026-06-02T07:25:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Serendipitous discovery of a bound nine-member protostellar system in NGC 6334-43 formed by filament fragmentation, with outflows from two sources and virial masses derived for three cores.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"2021), and outbursting protostars (e.g. V883 MNRAS000, 1-25 (2026) 6D. J. Taylor et al. Table 1.Properties of 1.20mm continuum sources Fitted properties Source Local𝜎 𝑎 S/N𝑎 Offset𝑏 Position (J2000)𝑏 I𝜈 𝑏 S𝜈 𝑏 Size𝑏 (mJy (mJy𝛼( h m s)𝛿( ◦ ′ ′′ )(mJy (mJy) (mas×mas [P.A.( ◦ ) ]) beam−1) beam −1) beam −1) ALMA1 0.499 281 - 17:20:23.60174−35:55:12.6999 139 (1) 266 (2) 272×228 [150] (3×3 [3]) ALMA2a𝑐 0.195 142 2.17 (0.04) 17:20:23.8439−35:54:56.449 24.2 (0.2) 35.9 (0.5) 211×152 [139] (7×8 [6]) ALMA2b𝑐 0.195 125 2.17 (0.04) 17:20:23.8596−35:54:56.873 22.4 (0.2) 29.9 (0.4) 169×139 [90] (7×6 [10]) ALMA2c𝑑 0.195 33 - 17:20:23.9878−35:54:56.52 - - 1310×980 [158] (30×20 [3]) ALMA3a𝑒 0.219 40 1.25 (0.02) 17:20:23.867 𝑒 −35:55:01.225𝑒 6."},{"citing_arxiv_id":"2606.00631","ref_index":18,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Ca-bearing cyanopolyynes in IRC+10216","primary_cat":"astro-ph.SR","submitted_at":"2026-05-30T09:06:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Abundance calculations for CaC_{2n+1}N (n=1-4) in IRC+10216 indicate observed CaNC originates from larger cyanopolyyne ions requiring molecular rearrangement during recombination.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13231","ref_index":61,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946","primary_cat":"astro-ph.GA","submitted_at":"2026-05-13T09:20:04+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"Hot cores in supernova remnant RX J1713.7-3946 exhibit column density ratios of complex organics, deuterated species, and S/N-bearing molecules that are indistinguishable from those in typical star-forming environments.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.08790","ref_index":14,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The evolution of C4H and c-C3H2 in molecular cores","primary_cat":"astro-ph.GA","submitted_at":"2026-05-09T08:21:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"C4H/H13CO+ and c-C3H2/H13CO+ abundance ratios decrease with molecular core evolution, indicating consumption of small unsaturated hydrocarbons into complex organic molecules.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05760","ref_index":135,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"ATOMIUM: Inner circumstellar envelopes of oxygen-rich AGB stars as revealed by highly excited SiO lines","primary_cat":"astro-ph.SR","submitted_at":"2026-05-07T06:55:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"ALMA Band 6 data detect SiO emission and masers up to v=8 in AGB stars, showing clumpy distributions, velocity gradients, and a tentative link between emission radius and mass-loss rate.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2601.22824","ref_index":49,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Rotational Spectroscopy as a Tool to Study Vibration-Rotation Interaction: Investigations of $^{13}$CH$_3$CN and CH$_3$$^{13}$CN up to $v_8 = 2$ and a Search for $v_8 = 2$ Transitions toward Sagittarius B2(N)","primary_cat":"astro-ph.GA","submitted_at":"2026-01-30T10:51:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"New spectroscopic measurements of 13CH3CN and CH3^13CN up to v8=2 yield precise l-component energy spacings of 22.93 and 21.79 cm^{-1} from perturbations and enable targeted searches in star-forming regions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2404.01044","ref_index":48,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Discovery of thionylimide, HNSO, in space: the first N-, S- and O-bearing interstellar molecule","primary_cat":"astro-ph.GA","submitted_at":"2024-04-01T10:57:08+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":9.0,"formal_verification":"none","one_line_summary":"First interstellar detection of HNSO with column density (8 ± 1)×10^13 cm^{-2} and abundance ~6×10^{-10} relative to H2, proposed to form via NSO + H on icy grains.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}