Distances to star forming regions
The determination of accurate distances to star-forming regions are discussed in the broader historical context of astronomical distance measurements. We summarize recent results for regions within 1 kpc and present perspectives for the near and more distance future.
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A detailed analysis of the Czernik 38 cluster and its associated tidal tail, utilizing Gaia DR3 and 2MASS. [PDF]
Ahmed NM.
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Lone black holes promise fresh insights into the fates of massive stars. [PDF]
Croswell K.
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How the characteristics of a virtual environment affects the perception of travel distance through it. [PDF]
Bansal A, McManus M, Harris LR.
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Using a neural network approach and starspots dependent models to predict effective temperatures and ages of young stars. [PDF]
Tarantino M +4 more
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Simulation of Dense Star Map in Deep Space Based on Gaia Catalogue. [PDF]
Li P, Bao G, Zhou Z, Gong J.
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Text embedding models yield detailed conceptual knowledge maps derived from short multiple-choice quizzes. [PDF]
Fitzpatrick PC, Heusser AC, Manning JR.
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Galaxy Evolution with Manifold Learning. [PDF]
Takeuchi TT, Cooray S, Kano RR.
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A large, long-lived, slowly-expanding superbubble across the Perseus arm. [PDF]
Chen B +7 more
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