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Related papers: Mid-Infrared Imaging of Young Stellar Objects

200 papers

We present new mid-infrared interferometric observations of the massive young stellar object IRAS 13481-6124, using VLTI/MIDI for spectrally-resolved, long-baseline measurements (projected baselines up to $\sim120$ m) and GSO/T-ReCS for…

The variability of Young Stellar Objects (YSOs) is a crucial tool for understanding the mechanisms driving flux changes. In this study, we present an infrared variability analysis of a large sample of over 20,000 candidate YSOs, using data…

Solar and Stellar Astrophysics · Physics 2025-03-19 Neha S. , Saurabh

We present an analysis of near-infrared time-series photometry in J, H, and K bands for about 100 epochs of a 1 square degree region of the Lynds 1003/1004 dark cloud in the Cygnus OB7 region. Augmented by data from the Wide-field Infrared…

Solar and Stellar Astrophysics · Physics 2015-06-16 Scott J. Wolk , Thomas S. Rice , Colin A. Aspin

Progress in understanding the embedded stars in LkHa225 has been hampered by their variability, making it hard to compare data taken at different times, and by the limited resolution of the available data, which cannot probe the small…

Deeply embedded and at distances of several kiloparsecs, massive young stellar objects (MYSOs) present numerous challenges for observation and study. In this work, we present spatially-resolved observations of one MYSO, AFGL 4176, together…

Solar and Stellar Astrophysics · Physics 2015-06-11 Paul Boley , Hendrik Linz , Roy van Boekel , Jeroen Bouwman , Thomas Henning , Andrey Sobolev

We found that at least 18 Young Stellar Object candidates invisible at optical and near-infrared wavelengths, as well as ^12CO emission. They are IRAS point sources with FIR colors similar to those of usual YSOs, and the infrared spectral…

Astrophysics · Physics 2015-06-24 Ikuru Iwata , Shin-ichiro Okumura , Mamoru Saito

Context. In multiple pre-main-sequence systems the lifetime of circumstellar disks appears to be shorter than around single stars, and the actual dissipation process may depend on the binary parameters of the systems. Aims. We report high…

Solar and Stellar Astrophysics · Physics 2017-07-12 Gergely Csépány , Mario van den Ancker , Péter Ábrahám , Rainer Köhler , Wolfgang Brandner , Felix Hormuth , Hector Hiss

We aim to characterize the distribution and composition of circumstellar material around young massive stars, and to investigate exactly which physical structures in these objects are probed by long-baseline mid-infrared interferometric…

We present high-resolution ($0\farcs2$) near-infrared images of the area surrounding the Herbig Be star LkH$\alpha$ 234 taken with the Coronagraphic Imager with Adaptive Optics (CIAO) and the adaptive optics on the Subaru Telescope. The…

Solar and Stellar Astrophysics · Physics 2015-05-28 Eri Kato , Misato Fukagawa , Marshall D. Perrin , Hiroshi Shibai , Yusuke Itoh , Takafumi Ootsubo

We report the discovery of a mid-infrared outburst in a Young Stellar Object (YSO) with an amplitude close to 8 mag at $\lambda$$\approx$4.6 $\mu$m. WISEA J142238.82-611553.7 is one of 23 highly variable WISE sources discovered in a search…

To study the demographics of interstellar ices in the Central Molecular Zone (CMZ) of the Milky Way, we obtain near-infrared spectra of $109$ red point sources using NASA IRTF/SpeX at Maunakea. We select the sample from near- and…

Astrophysics of Galaxies · Physics 2022-05-11 Dajeong Jang , Deokkeun An , Kris Sellgren , Solange V. Ramírez , A. C. Adwin Boogert , Mathias Schultheis

We report the results of a spectroscopic survey of 20 close T Tauri binaries in the Taurus-Auriga dark cloud where the separations between primaries and their secondaries are less than the typical size of a circumstellar disk around a young…

Astrophysics · Physics 2009-11-07 Patrick Hartigan , Scott Kenyon

Due to the recent dramatic technological advances, infrared interferometry can now be applied to new classes of objects, resulting in exciting new science prospects, for instance, in the area of high-mass star formation. Although…

We present new mid-IR observations of the quadruply lensed quasar Q2237+0305 taken with CanariCam on the Gran Telescopio Canarias. Mid-IR emission by hot dust, unlike the optical and near-IR emission from the accretion disk, is unaffected…

Astrophysics of Galaxies · Physics 2016-11-21 H. Vives-Arias , J. A. Munoz , C. S. Kochanek , E. Mediavilla , J. Jimenez-Vicente

We present the first Spitzer Infrared Spectrograph (IRS; The IRS was a collaborative venture between Cornell University and Ball Aerospace Corporation funded by NASA through the Jet Propulsion Laboratory and the Ames Research Center.)…

Using photometric data of infrared surveys, young stellar object (YSO) status is verified for 141 objects selected in our previous papers in the Cassiopeia and Camelopardalis segment of the Milky Way bounded by Galactic coordinates (l, b) =…

Solar and Stellar Astrophysics · Physics 2018-03-14 V. Straizys , A. Kazlauskas

We present a catalog of 167 newly discovered, irregular variables spanning a $\sim$7 deg${^2}$ area that encompasses the G 305 star-forming complex, one of the most luminous giant H II regions in the Galaxy. We aim to unveil and…

Aims: We present mid-infrared observations and photometry of the transitional disks around the young stellar objects DH Tau, DM Tau, and GM Aur, obtained with VISIR/VLT in N band. Our aim is to resolve the inner region and the large-scale…

Solar and Stellar Astrophysics · Physics 2015-05-30 Christian Gräfe , Sebastian Wolf , Veronica Roccatagliata , Jürgen Sauter , Steve Ertel

We use various analytical techniques to study Young Stellar Objects (YSOs) in an area of approximately $10' \times 10'$ in the IRAS 18456-0223 star-forming region. We use archival optical (Gaia DR3) and infrared (2MASS, UKIDSS, Spitzer,…

Solar and Stellar Astrophysics · Physics 2026-03-06 Nilesh Pandey , U. S. Kamath

The young binary system T Tau was observed with the Owens Valley Millimeter Array at 267 GHz continuum and HCO+ J=3-2 emission at 0.8'' resolution, with the JCMT-CSO single-baseline interferometer in 357 GHz continuum, and with the W. M.…