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相关论文: UYSO 1 - An Extremely Young Massive Stellar Object

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The theory of massive star formation currently suffers from a scarce observational base of massive young stellar objects to compare with. In this paper, we present OVRO CO(1-0), 13CO(1-0), C18O(1-0), and 2.6 mm continuum images of the…

The results of the searching on the bases of GPS UKIDSS survey's data of dense compact stellar clusters in the vicinity of 20 YSOs with high and middle masses are presented. Totally we have revealed clusters in 13 areas. Around 5 objects…

太阳与恒星天体物理 · 物理学 2015-12-29 N. M. Azatyan , E. H. Nikoghosyan

We report the detection of several molecular gas-phase and ice absorption features in three photometrically-selected young stellar object (YSO) candidates in the central 280 pc of the Milky Way. Our spectra, obtained with the Infrared…

IRAS 23385+6053 is a Young Stellar Object with luminosity 16,000 solar luminosities at a kinematic distance of 4.9 kpc. This candidate precursor of an ultracompact HII region is associated with a millimeter source detected at the JCMT but…

天体物理学 · 物理学 2009-10-30 Sergio Molinari , Leonardo Testi , Jan Brand , Riccardo Cesaroni , Francesco Palla

We present the results of CS J=2-1 mapping observations towards 39 massive star-forming regions selected from the previous CO line survey of cold IRAS sources with high-velocity CO flows along the Galactic plane (Yang et al. 2002). All…

太阳与恒星天体物理 · 物理学 2018-11-14 Yiping Ao , Ji Yang , Kenichi Tatematsu , Christian Henkel , Kazuyoshi Sunada , Quang Nguyen-Luong

IRAS 19312+1950 is a peculiar object that has eluded firm characterization since its discovery, with combined maser properties similar to an evolved star and a young stellar object (YSO). To help determine its true nature, we obtained…

The very inner structure of massive young stellar objects (YSOs) is difficult to trace. With conventional observational methods we identify structures still several hundreds of AU in size. However, the (proto-)stellar growth takes place at…

天体物理学 · 物理学 2014-11-18 H. Linz , B. Stecklum , R. Follert , Th. Henning , R. van Boekel , A. Men'shchikov , I. Pascucci , M. Feldt

We present a multiwavelength study towards the young stellar object (YSO) G29.862-0.044 (hereafter G29), which is embedded in the massive star-forming region G29.96-0.02, located at a distance of about 6.5 kpc. The surrounding interstellar…

星系天体物理 · 物理学 2019-04-25 M. B. Areal , S. Paron , M. E. Ortega , C. Fariña

Aims: We aim to understand the star formation associated with the luminous young stellar object (YSO) IRAS 18345-0641 and to address the complications arising from unresolved multiplicity in interpreting the observations of massive…

太阳与恒星天体物理 · 物理学 2015-06-15 Watson P. Varricatt , Holly S. Thomas , Chris J. Davis , Suzanne Ramsay , Malcolm J. Currie

We report the discovery of a new young stellar cluster and molecular cloud located in the far outer Galaxy, seen towards IRAS 06361-0142, and we characterise their properties. Near-infrared images were obtained with VLT/ISAAC through JHKs…

天体物理学 · 物理学 2019-08-19 Joao L. Yun , Ana Lopez-Sepulcre , Jose M. Torrelles

We describe an object in the Hubble Deep Field North with very unusual near-infrared properties. It is readily visible in Hubble Space Telescope NICMOS images at 1.6um and from the ground at 2.2um, but is undetected (with signal-to-noise <~…

Massive stars are rarely seen to form in isolation. It has been proposed that association with companions or clusters in the formative stages is vital to their mass accumulation. In this paper we study IRAS~18144-1723, a massive young…

太阳与恒星天体物理 · 物理学 2018-08-08 W. P. Varricatt , J. G. A. Wouterloot , S. K. Ramsay , C. J. Davis

We present the initial results of our investigation of the star-forming complex W49, one of the youngest and most luminous massive star forming regions in our Galaxy. We used Spitzer/Infrared Array Camera (IRAC) data to investigate massive…

太阳与恒星天体物理 · 物理学 2015-12-17 Gozde Saral , Joseph L. Hora , Sarah E. Willis , Xavier P. Koenig , Robert A. Gutermuth , A. Talat Saygac

The optically invisible infrared-source NGC 2264 IRS 1 is thought to be a massive young stellar object (~10 Msun). Although strong infrared excess clearly shows that the central object is surrounded by large amounts of circumstellar…

太阳与恒星天体物理 · 物理学 2015-05-28 R. Grellmann , Th. Ratzka , S. Kraus , H. Linz , Th. Preibisch , G. Weigelt

We report the discovery of two very cold and massive molecular cloud cores in the region ISOSS J18364-0221. The object has been identified by a systematic search for very early evolutionary stages of high-mass stars using the 170 micron…

天体物理学 · 物理学 2016-08-30 Stephan M. Birkmann , Oliver Krause , Dietrich Lemke

Jets and outflows from Young Stellar Objects (YSOs) are important signposts of currently ongoing star formation. In order to study these objects we are conducting an unbiased survey along the Galactic Plane in the 1-0S(1) emission line of…

星系天体物理 · 物理学 2015-06-03 G. Ioannidis , D. Froebrich

G79.3+0.3 is an infrared dark cloud in the Cygnus-X complex that is home to massive deeply embedded young stellar objects (YSOs). We have produced a submillimeter array (SMA) 1.3 mm continuum image and $^{12}$CO line maps of the eastern…

太阳与恒星天体物理 · 物理学 2019-05-15 Anna S. E. Laws , Joseph L. Hora , Qizhou Zhang

Using the infrared photometry data extracted from the 2MASS, IRAS and MSX databases, 50 suspected young stellar objects (YSOs) are selected from about 37500 infrared objects in the 3x3 deg area with the center at Galactic longitude 142.5…

天体物理学 · 物理学 2009-06-25 V. Straizys , V. Laugalys

We have carried out near-infrared spectroscopic observations of 23 very low-luminosity young stellar object (YSO) candidates and 5 their companions in Heiles Cloud 2, one of the densest parts of the Taurus molecular cloud. Twelve objects…

天体物理学 · 物理学 2015-06-24 Y. Itoh , M. Tamura , A. Tokunaga

The study of Young Stellar Objects (YSOs) is one of the most exciting topics that can be undertaken by long baseline optical interferometry. The magnitudes of these objects are at the edge of capabilities of current optical interferometers,…

天体物理学 · 物理学 2009-11-07 Fabien Malbet