Q-FEEDBACK-MULTIPHASE-COUPLING · provisional_seed
超新星、恒星风、辐射、AGN辐射与喷流驱动的冷—暖—热多相气体响应及跨尺度传输。
仅判断宿主是否有AGN而没有气体响应测量的论文。
决定星系形成模型中的重子循环、淬火和金属富集是否具有可验证的物理闭合。
Dissecting the Nuclear Structure of NGC 5548 with XRISM. I. Physical Properties of the Highly Ionized Outflows
deterministic_keyword_v1_1 · confidence=0.55
The outflow's mass loading factor is ~2, suggesting that stellar feedback could remove the remaining gas on timescales shorter than those required for depletion by star formation alone.
deterministic_keyword_v1 · confidence=0.63
Arkenstone is a subgrid framework for representing multiphase flows in coarse resolution simulations that has been used to model stellar feedback driven galactic winds.
deterministic_keyword_v1 · confidence=0.67
The mass and energetics of this distant outflow are consistent with nearby starburst-driven superwinds, suggesting that the efficiency of stellar feedback has remained relatively constant over the last 12 billion years of cosmic history.
deterministic_keyword_v1 · confidence=0.63
Increased flux at energies ≳ 41 eV suggests that the compact gas structures experience an additional harder ionizing radiation source, which is most likely driven by localized fast radiative shocks from stellar winds, a hypothetical Sgr A* outflow, and/or interactions with the ambient medium.
deterministic_keyword_v1 · confidence=0.55
The molecular gas is only weakly coupled to the stellar feedback that dominates the ionized phase.
deterministic_keyword_v1 · confidence=0.59
The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the L_X–T relation of early-type galaxies
deterministic_keyword_v1 · confidence=0.55