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相关论文: New light on the S235A-B star forming region

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We report on new aspects of the star-forming region S235AB revealed through high-resolution observations at radio and mid-infrared wavelengths. Using the Very Large Array, we carried out sensitive observations of S235AB in the cm continuum…

天体物理学 · 物理学 2009-11-11 Marcello Felli , Fabrizio Massi , Massimo Robberto , Riccardo Cesaroni

We present the {\it Spitzer}-IRAC images of the S235 star forming complex that includes the East~1 & 2, Central and S235 A & B regions. In addition, we present the near-infrared images of the S235 A & B regions. The IRAC photometry reveals…

星系天体物理 · 物理学 2015-05-27 L. K. Dewangan , B. G. Anandarao

In this paper an extensive survey of the star forming complex Sh2-252 has been undertaken with an aim to explore its hidden young stellar population as well as to understand the structure and star formation history. This complex is composed…

太阳与恒星天体物理 · 物理学 2015-06-15 Jessy Jose , A. K. Pandey , M. R. Samal , D. K. Ojha , K. Ogura , J. S. Kim , N. Kobayashi , A. Goyal , N. Chauhan , C. Eswaraiah

We present radio and infrared observations indicating on-going star formation activity inside the $\sim2-5$ pc circumnuclear ring at the Galactic center. Collectively these measurements suggest a continued disk-based mode of on-going star…

We have carried out an extensive multi-wavelength study to investigate the star formation process in the S235 complex. The S235 complex has a sphere-like shell appearance at wavelengths longer than 2 $\mu$m and harbors an O9.5V type star…

星系天体物理 · 物理学 2016-03-16 L. K. Dewangan , D. K. Ojha , A. Luna , B. G. Anandarao , J. P. Ninan , K. K. Mallick , Y. D. Mayya

(abridged) We study a previously discovered protostellar source that is deeply embedded and drives an energetic molecular outflow. The source, UYSO1, is located close to IRAS 07029-1215 at a distance of ~1 kpc. The multi-wavelength…

This work aims at investigating the molecular gas component in the vicinity of two young stellar object (YSO) candidates identified at the border of the HII region G034.8-0.7 that is evolving within a molecular cloud shocked by the SNR W44.…

星系天体物理 · 物理学 2015-05-13 S. Paron , M. E. Ortega , M. Rubio , G. Dubner

We used the Very Long Baseline Array (VLBA) and the European VLBI Network (EVN) to perform phase-referenced VLBI observations of the three most powerful maser transitions associated with the high-mass star-forming region G28.87+0.07: the…

太阳与恒星天体物理 · 物理学 2015-06-03 J. J. Li , L. Moscadelli , R. Cesaroni , R. S. Furuya , Y. Xu , T. Usuda , K. M. Menten , M. Pestalozzi , D. Elia , E. Schisano

We present a multi-wavelength analysis of a $\sim$30$' \times$30$'$ area around the Sh 2-53 region (hereafter S53 complex), which is associated with at least three H II regions, two mid-infrared bubbles (N21 and N22), and infrared dark…

星系天体物理 · 物理学 2018-01-31 T. Baug , L. K. Dewangan , D. K. Ojha , Kengo Tachihara , A. K. Pandey , Saurabh Sharma , M. Tamura , J. P. Ninan , S. K. Ghosh

High-mass star formation is not well understood chiefly because examples are deeply embedded, relatively distant, and crowded with sources of emission. Using VLA and VLBA observations of water and SiO maser emission, we have mapped in…

天体物理学 · 物理学 2007-05-23 L. J. Greenhill , M. J. Reid , C. J. Chandler , P. J. Diamond , M. Elitzur

We present results of continuum and spectral line observations with ALMA and 22 GHz water (H$_2$O) maser observations using KaVA and VERA toward a high-mass star-forming region, G25.82-0.17. Multiple 1.3 mm continuum sources are revealed,…

We present a multi-wavelength study to analyse the star formation process associated with the mid-infrared bubble CN 148 (H II region G10.3-0.1), which harbors an O5V-O6V star. The arc-shaped distribution of molecular CO(2-1) emission, the…

星系天体物理 · 物理学 2015-06-23 L. K. Dewangan , D. K. Ojha , J. M. C. Grave , K. K. Mallick

(abbreviated) In the central part of the S254-S258 star forming complex, a dense embedded cluster of very young stellar objects (S255-IR) is sandwiched between the two HII regions S255 and S257. This interesting configuration had led to…

星系天体物理 · 物理学 2015-05-28 Paola Mucciarelli , Thomas Preibisch , Hans Zinnecker

We investigate at a high angular resolution the spatial and kinematic structure of the S255IR high mass star-forming region, which demonstrated recently the first disk-mediated accretion burst in the massive young stellar object. The…

星系天体物理 · 物理学 2020-02-05 Igor I. Zinchenko , Sheng-Yuan Liu , Yu-Nung Su , Kuo-Song Wang , Yuan Wang

Our aim is to investigate the protostellar jets inside the young stellar object (YSO) cluster G105.42+9.88 (alias LkH$\alpha$ 234). This is one of the least luminous targets of the Protostellar Outflows at the EarliesT Stages (POETS)…

太阳与恒星天体物理 · 物理学 2025-08-06 Luca Moscadelli , Fabrizio Massi , Olga Bayandina

We present a picture of star formation around the HII region Sh2-235 (S235) based upon data on the spatial distribution of young stellar clusters and the distribution and kinematics of molecular gas around S235. We observed 13CO(1-0) and…

天体物理学 · 物理学 2009-11-13 M. S. Kirsanova , A. M. Sobolev , M. Thomasson , D. S. Wiebe , L. E. B. Johansson , A. F. Seleznev

The connection between high-mass stars and young stellar clusters has been well established by near-IR observations showing young massive stars in HII regions surrounded by clusters of lower mass stars. Mm-wave observations show that these…

天体物理学 · 物理学 2007-05-23 A. R. Tieftrunk , S. T. Megeath , S. Thorwirth

Context. The S235AB star forming region houses a massive young stellar object which has recently been reported to exhibit possible evidence of jet rotation - an illusive yet crucial component of disk aided star formation theories. Aims. To…

太阳与恒星天体物理 · 物理学 2016-01-27 R. A. Burns , T. Handa , T. Hirota , K. Motogi , I. Imai , T. Omodaka

S255N is a luminous far-infrared source that contains many indications of active star formation but lacks a prominent near-infrared stellar cluster. We present mid-infrared through radio observations aimed at exploring the evolutionary…

天体物理学 · 物理学 2009-06-23 C. J. Cyganowski , C. L. Brogan , T. R. Hunter

We present a multi-wavelength observational study of a low-mass star-forming region, L1251-C, with observational results at wavelengths from the near-infrared to the millimeter. Spitzer Space Telescope observations confirmed that IRAS…

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