New catalogue of 1423 Gaia DR3 variable white dwarf candidates, with 141 ZTF-confirmed periodic variables classified into known types and 83 newly identified periodic stars.
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3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.SR 3representative citing papers
Pismis 18 is an intermediate-age (~700 Myr) inner-disc open cluster at ~7 kpc Galactocentric distance with [Fe/H] = +0.23, slightly super-solar [α/Fe] and s-process elements, and updated parameters from high-confidence members.
VLBA astrometry measures parallaxes of 2.26-2.65 mas for YSOs in Orion, determining mean distances of 405 pc for NGC 2068, 403 pc for NGC 2024, 407 pc for sigma Orionis, 388.5 pc for the ONC, and 438 pc for L1641.
citing papers explorer
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Gaia DR3 Variable White Dwarfs vetted by ZTF
New catalogue of 1423 Gaia DR3 variable white dwarf candidates, with 141 ZTF-confirmed periodic variables classified into known types and 83 newly identified periodic stars.
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The Gaia-ESO Survey: The inner disc, intermediate-age open cluster Pismis 18
Pismis 18 is an intermediate-age (~700 Myr) inner-disc open cluster at ~7 kpc Galactocentric distance with [Fe/H] = +0.23, slightly super-solar [α/Fe] and s-process elements, and updated parameters from high-confidence members.
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Dynamical masses of YSOs with the VLBA: DYNAMO VLBA: Trigonometric parallaxes and proper motions of YSOs in Orion
VLBA astrometry measures parallaxes of 2.26-2.65 mas for YSOs in Orion, determining mean distances of 405 pc for NGC 2068, 403 pc for NGC 2024, 407 pc for sigma Orionis, 388.5 pc for the ONC, and 438 pc for L1641.