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The UV Perspective of Low-Mass Star Formation
DOI: 10.3390/galaxies8010027 Bibcode: 2020Galax...8...27S

France, Kevin; Schneider, P. Christian; Günther, H. Moritz

The formation of low-mass (M★≲2M⊙) stars in molecular clouds involves accretion disks and jets, which are of broad astrophysical interest. Accreting stars represent the closest examples of these phenomena. Star and planet formation are also intimately connected, setting the starting point for planetary systems like our own. The ultraviolet (UV) sp…

2020 Galaxies
eHST 15
Massive Star Formation in the Ultraviolet Observed with the Hubble Space Telescope
DOI: 10.3390/galaxies8010013 Bibcode: 2020Galax...8...13L

Leitherer, Claus

Spectroscopic observations of a massive star formation in the ultraviolet and their interpretation are reviewed. After a brief historical retrospective, two well-studied resolved star clusters and the surrounding H II regions are introduced: NGC 2070 in the Large Magellanic Cloud and NGC 604 in M33. These regions serve as a training set for studie…

2020 Galaxies
eHST 12
Unraveling the Physics of Quasar Jets: Optical Polarimetry and Implications for the X-ray Emission Process
DOI: 10.3390/galaxies8040071 Bibcode: 2020Galax...8...71P

Perlman, Eric S.; Clautice, Devon; Avachat, Sayali +4 more

Since the launch of Chandra twenty years ago, one of the greatest mysteries surrounding Quasar Jets is the production mechanism for their extremely high X-ray luminosity. Two mechanisms have been proposed. In the first view, the X-ray emission is inverse-Comptonized CMB photons. This view requires a jet that is highly relativistic (bulk Lorentz fa…

2020 Galaxies
eHST 10
First Results from a Panchromatic HST/WFC3 Imaging Study of the Young, Rapidly Evolving Planetary Nebulae NGC 7027 and NGC 6302
DOI: 10.3390/galaxies8020049 Bibcode: 2020Galax...8...49K

Frank, Adam; Balick, Bruce; Kastner, Joel H. +3 more

We present the first results from comprehensive, near-UV-to-near-IR Hubble Space Telescope Wide Field Camera 3 (WFC3) emission-line imaging studies of two young planetary nebulae (PNe), NGC 7027 and NGC 6302. These two objects represent key sources for purposes of understanding PNe shaping processes. Both nebulae feature axisymmetric and point-sym…

2020 Galaxies
eHST 5
On the Age of Galactic Bulge CSPNe: Too Young and Complicated?
DOI: 10.3390/galaxies8020051 Bibcode: 2020Galax...8...51L

Parker, Quentin A.; Lykou, Foteini; Zijlstra, Albert

We present preliminary results of our study of a small sample of planetary nebulae in the Galactic Bulge for which high-angular resolution Hubble Space Telescope imaging is available. From this and from archival spectroscopy, we were able to calculate temperatures and luminosities for their central stars. These were then correlated to up-to-date e…

2020 Galaxies
Gaia eHST 0