▪ Abstract Stellar clusters are born embedded within giant molecular clouds (GMCs) and
during their formation and early evolution are often only visible at infrared wavelengths …

Understanding the formation of stars in galaxies is central to much of modern astrophysics.
However, a quantitative prediction of the star formation rate and the initial distribution of …

The nature and origin of free-floating planets (FFPs) are still largely unconstrained because
of a lack of large homogeneous samples to enable a statistical analysis of their properties …

ABSTRACT We present a 0.8–5 μm spectral library of 210 cool stars observed at a resolving
power of R≡ λ/Δλ∼ 2000 with the medium-resolution infrared spectrograph, SpeX, at the …

Context. Understanding how star formation begins and propagates through molecular
clouds is a fundamental but still open question. One major difficulty in addressing this …

We present the results of an extensive 1.3 mm continuum mosaicing study of the rho
Ophiuchi central region obtained at the IRAM 30-m telescope with the MPIfR 19-channel …

On the Stellar Population and Star-Forming History of the Orion Nebula Cluster ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

We re-examine the observed near-infrared properties of T Tauri stars and interpret them with
the aid of accretion disk models. Based upon a careful analysis of the dereddened near …

Recent discoveries of extrasolar planets and new direct evidence for protoplanetary disks
around young stars have had a major impact on our understanding of star and planet …

We present a high spatial resolution submillimeter continuum survey of 24 circumstellar
disks in the Taurus-Auriga and Ophiuchus-Scorpius star formation regions using the SMA. In …