Abstract The Vera C. Rubin Legacy Survey of Space and Time (LSST) holds the potential to
revolutionize time domain astrophysics, reaching completely unexplored areas of the …

The clusters of young stars in massive star-forming regions show a wide range of sizes,
morphologies, and numbers of stars. Their highly subclustered structures are revealed by …

Solar-type stars exhibit their highest levels of magnetic activity during their early convective
pre-main-sequence (PMS) phase of evolution. The most powerful PMS flares, superflares …

ABSTRACT The Massive Young Star-Forming Complex Study in Infrared and X-ray (MYStIX)
seeks to characterize 20 OB-dominated young clusters and their environs at distances d⩽ 4 …

Within 40 years of the detection of the first extra-solar x-ray source in 1962, NASA's Chandra
X-ray Observatory has achieved an increase in sensitivity of 10 orders of magnitude …

Abstract Vera C. Rubin Observatory, through the Legacy Survey of Space and Time (LSST),
will allow us to derive a panchromatic view of variability in young stellar objects (YSOs) …

Star clusters larger than∼ 103 M⊙ contain multiple hot stars that launch fast stellar winds.
The integrated kinetic energy carried by these winds is comparable to that delivered by …

We present a catalog of 1439 young stellar objects (YSOs) spanning the 1.42 deg 2 field
surveyed by the Chandra Carina Complex Project (CCCP), which includes the major …

The key empirical property of the X-ray emission from O stars is a strong correlation between
the bolometric and X-ray luminosities. In the framework of the Chandra Carina Complex …

Context. The Carina Nebula complex (CNC) is one of the most massive and active star-
forming regions in our Galaxy and it contains several large young star clusters. The …