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Using GALEX-SDSS-PanSTARRS-HST-Gaia to understand post-AGB evolution
DOI: 10.1007/s10509-018-3369-z Bibcode: 2018Ap&SS.363..166B

Bianchi, Luciana; Casewell, Sarah; Bohlin, Ralph +2 more

Hot WDs in binary systems with a less evolved star are particularly invaluable astrophysical probes, the unevolved companion enabling better derivation of distance and age than is usually possible for post-AGB objects, and therefore also of their radius and luminosity. But hot white dwarfs (WD) are elusive at all wavelengths except the UV (Bianchi…

2018 Astrophysics and Space Science
Gaia eHST 8
History of globulettes in the Milky Way
DOI: 10.1007/s10509-017-3233-6 Bibcode: 2018Ap&SS.363...28G

Grenman, Tiia; Elfgren, Erik; Weber, Hans

Globulettes are small (radii <10 kAU) dark dust clouds, seen against the background of bright nebulae. A majority of the objects have planetary mass. These objects may be a source of brown dwarfs and free floating planetary mass objects in the gala…

2018 Astrophysics and Space Science
eHST 2