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Related papers: A systematic survey for eruptive young stellar obj…

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Photometric variability in young stellar objects (YSOs) provides critical insight into the mechanisms of mass accretion, disk evolution, and circumstellar extinction in early stellar evolution. We present an analysis of day-timescale…

Current planet formation models are largely based on the observational constraint that protoplanetary disks have lifetime 3Myr. Recent studies, however, report the existence of PMS stars with signatures of accretion (strictly connected with…

Solar and Stellar Astrophysics · Physics 2015-06-16 C. F. Manara , G. Beccari , N. Da Rio , G. De Marchi , A. Natta , L. Ricci , M. Robberto , L. Testi

High resolution (lambda / Delta-lambda = 50,000) K-band spectra of massive, embedded, young stellar objects are presented. The present sample consists of four massive young stars located in nascent clusters powering Galactic giant H II…

Astrophysics · Physics 2009-11-10 R. D. Blum , C. L. Barbosa , A. Damineli , P. S. Conti , S. Ridgway

We report the results of a recent study of young star clusters (YSCs) in luminous blue compact galaxies (BCGs). The age distributions of the YSCs suggest that the starburst episode in Haro 11, ESO 185-IG13, and Mrk 930 started not more than…

Cosmology and Nongalactic Astrophysics · Physics 2011-07-05 Angela Adamo , Goeran Ostlin , Erik Zackrisson

Stars may be assembled in large growth spurts, however the evidence for this hypothesis is circumstantial. Directly studying the accretion at the earliest phases of stellar growth is challenging because young stars are deeply embedded in…

Solar and Stellar Astrophysics · Physics 2015-06-12 Doug Johnstone , Benjamin Hendricks , Gregory J. Herczeg , Simon Bruderer

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 luminous Young Stellar Object (YSO) IRAS 07422-2001 is studied in the infrared. We discover star forming activity in embedded clusters located in a cloud detected at mid-IR wavelengths in emission. Multiple outflows are discovered from…

Solar and Stellar Astrophysics · Physics 2015-06-04 Watson P. Varricatt

Jets and outflows accompany the mass accretion process in protostars and young stellar objects. Using a large and unbiased sample, they can be used to study statistically the local feedback they provide and the typical mass accretion…

Astrophysics of Galaxies · Physics 2015-06-05 G. Ioannidis , D. Froebrich

Results of a comprehensive, new, ground-based mid-infrared imaging survey of the young stellar population of the Rho Ophiuchi cloud are presented. Data were acquired at the Palomar 5-m and at the Keck 10-m telescopes with the MIRLIN and LWS…

Astrophysics · Physics 2009-11-11 Mary Barsony , Michael E. Ressler , Kenneth A. Marsh

We discuss accretion and outflow properties of three very low-mass young stellar objects based on broad-band mid-resolution X-Shooter/VLT spectra. Our targets (FU TauA, 2M 1207-39, and Par-Lup3-4) have spectral types between M5 and M8, ages…

Solar and Stellar Astrophysics · Physics 2015-06-17 B. Stelzer , J. M. Alcala , E. Whelan , A. Scholz

We present an analytical study of a large sample of ~109 young stellar objects in the X-ray. Our objects were detected in X-ray independent of age. Unexpectedly, the X-ray energy is somewhat correlated with the ages. It decreases with time…

Solar and Stellar Astrophysics · Physics 2015-03-17 M. Hamidouche , M. Jacobson , L. W. Looney

We present Submillimeter Array observations of the young stellar object IRAS 04579+4703 in the 1.3 mm continuum and in the 12CO(2-1), 13CO(2-1) and C18O(2-1) lines. The 1.3 mm continuum image reveals a flattened structure with a mass of 13…

Solar and Stellar Astrophysics · Physics 2015-06-04 Jin-Long Xu , Jun-Jie Wang , Sheng-Li Qin

We present Spitzer IRAC images that indicate the presence of cavities cut into the dense outer envelope surrounding very young pre-main sequence stars. These young stellar objects (YSOs) characterized by an outflow represent the earliest…

Astrophysics · Physics 2007-11-28 Jonathan P. Seale , Leslie W. Looney

A small subset of young stellar objects (YSOs) exhibit "see-saw" temporal variations in their mid-infrared SED; as the flux short-ward of a fulcrum wavelength ($\lambda_{f}$) increases the flux long-wards of this wavelength decreases (and…

Earth and Planetary Astrophysics · Physics 2019-09-25 Geoffrey R. Bryan , Sarah T. Maddison , Kurt Liffman

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 report on the ongoing outburst of the young variable V1180 Cas, which is known to display characteristics in common with EXor eruptive variables. We present results that support the scenario of an accretion-driven nature of the…

We present an IR-monitoring survey with the $Spitzer$ Space Telescope of the star forming region GGD 12-15. Over 1000 objects were monitored including about 350 objects within the central 5 arcminutes which is found to be especially dense…

We report on the results of an optical spectroscopic survey designed to confirm the youth and determine the spectral types among a sample of young stellar object (YSO) candidates in the Serpens Molecular Cloud. We observed 150 infrared…

The $K2$ Mission has photometrically monitored thousands of stars at high precision and cadence in a series of $\sim$80-day campaigns focused on sections of the ecliptic plane. During its second campaign, $K2$ targeted over 1000 young…

Solar and Stellar Astrophysics · Physics 2018-08-08 Ann Marie Cody , Lynne A. Hillenbrand

We have made 12CO 2-1 and 1-0 maps of eleven molecular outflows associated with intermediate to high-mass young stellar objects (YSOs) in order to establish whether the correlations between outflow parameters and source bolometric…

Astrophysics · Physics 2009-11-07 Naomi A. Ridge , Toby J. T. Moore