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Related papers: A young bipolar outflow from IRAS 15398-3359

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We present observations and analysis of the massive molecular outflow G331.512-0.103, obtained with ALMA band 7, continuing the work from Merello et al. (2013). Several lines were identified in the observed bandwidth, consisting of two…

Resolving physical and chemical structures in the vicinity of a protostar is of fundamental importance for elucidating their evolution to a planetary system. In this context, we have conducted 1.2 mm observations toward the low-mass…

Astrophysics of Galaxies · Physics 2022-08-31 Yuki Okoda , Yoko Oya , Muneaki Imai , Nami Sakai , Yoshimasa Watanabe , Ana López-Sepulcre , Kazuya Saigo , Satoshi Yamamoto

It is not well known what drives the chemistry of a protostellar envelope, in particular the role of the stellar mass and the outflows on its chemical enrichment. We study the chemical structure of NGC 1333 IRAS 4A in order to (i)…

Astrophysics of Galaxies · Physics 2017-07-12 E. Koumpia , D. A. Semenov , F. F. S. van der Tak , A. C. A. Boogert , E. Caux

As part of the ALMA Large Program "Early Planet Formation in Embedded Disks" (eDisk), 12CO (2 - 1) was observed towards 19 nearby low-mass protostars. Of these objects, 15 sources are found to show molecular outflow emission. Based on their…

Using the ASTE 10 m submillimeter telescope and the 1.4 m Infrared Survey Facility (IRSF), we performed an extensive outflow survey in the Orion Molecular Cloud -2 and -3 region. Our survey, which includes 41 potential star-forming sites,…

We present results from three-dimensional, self-gravitating, radiation-hydrodynamic simulations of low-mass protostellar outflows. We construct synthetic observations in 12CO in order to compare with observed outflows and evaluate the…

Solar and Stellar Astrophysics · Physics 2015-05-30 S. S. R. Offner , E. J. Lee , A. A. Goodman , H. Arce

We present an analysis of the molecular and atomic gas emission in the rest-frame far-infrared and sub-millimetre, from the lensed z=2.3 sub-millimetre galaxy SMM J2135-0102. We obtain very high signal-to-noise detections of 11 transitions…

This paper presents a large spectral line and continuum survey of 8 deeply embedded, low-mass protostellar cores using the Submillimeter Array. Each source was observed in high excitation lines of some of the most common molecular species,…

A massive envelope and a strong bipolar outflow are the two main structures characterizing the youngest protostellar systems. In order to understand the physical properties of a bipolar outflow and the relationship with those of the…

Solar and Stellar Astrophysics · Physics 2015-10-09 Woojin Kwon , Manuel Fernandez-Lopez , Ian W. Stephens , Leslie W. Looney

We present and discuss \emph{Spitzer} and near-infrared H$_{2}$ observations of a new bi-polar protostellar outflow in the Rosette Molecular Cloud. The outflow is seen in all four IRAC bands and partially as diffuse emission in the MIPS 24…

Solar and Stellar Astrophysics · Physics 2015-05-18 Jason E. Ybarra , Elizabeth A. Lada , Zoltan Balog , Scott W Fleming , Randy L. Phelps

Direct observations of accretion disks around high-mass young stellar objects would help to discriminate between different models of formation of massive stars. However, given the complexity of massive star forming regions, such studies are…

Solar and Stellar Astrophysics · Physics 2015-05-27 S. Leurini , C. Codella , L. Zapata , M. T. Beltran , P. Schilke , R. Cesaroni

To shed light on the early phase of a low-mass protostar formation process, we conducted interferometric observations towards a protostar GF9-2 using the CARMA and SMA. The observations have been carried out in the CO J=3-2 line and in the…

Astrophysics of Galaxies · Physics 2022-10-05 Ray S. Furuya , Yoshimi Kitamura , Hiroko Shinnaga

We present SO and SO2 observations in the region of the low mass protostar IRAS2/NGC1333. The East-West outflow originating from this source has been mapped in four transitions of both SO and SO2. In addition, CS observations published in…

We present the first detection of spatially resolved protostellar outflows and jets in the outer Galaxy. We observed five star-forming regions in the outer Galaxy (Sh 2--283, NOMF05-16/19/23/63; galactocentric distance = 15.7--17.4 kpc)…

We examine emission from a young protostellar object (YPO) with three-dimensional ideal MHD simulations and three-dimensional non-local thermodynamic equilibrium (non-LTE) line transfer calculations, and show the first results. To calculate…

Solar and Stellar Astrophysics · Physics 2015-05-13 M. Yamada , M. N. Machida , S. Inutsuka , K. Tomisaka

We have carried out high-angular resolution (1.4") observations in the continuum at 3.1mm and in the N2H+ 1-0, CH3CN 5_k-4_k and 13CS 2-1 lines using the Plateau de Bure Interferometer (PdBI) towards the intermediate mass (IM) protostar…

Astrophysics of Galaxies · Physics 2015-05-14 A. Fuente , A. Castro-Carrizo , T. Alonso-Albi , M. T. Beltran , R. Neri , C. Ceccarelli , B. Lefloch , C. Codella , P. Caselli

This paper investigates small-scale structures of dense gas and dust around the low-mass protostellar binary NGC1333-IRAS2 using millimeter-wavelength aperture-synthesis observations from the OVRO and BIMA interferometers. The detected 3 mm…

Episodic accretion plays an important role in the evolution of young stars. Although it has been under investigation for a long time, the origin of such episodic accretion events is not yet understood. We investigate the dust and gas…

Solar and Stellar Astrophysics · Physics 2019-10-16 Andreas Postel , Marc Audard , Eduard Vorobyov , Odysseas Dionatos , Christian Rab , Manuel Güdel

During the embedded stage of star formation, bipolar molecular outflows and UV radiation from the protostar are important feedback processes. Our aim is to quantify the feedback, mechanical and radiative, for a large sample of low-mass…

We present sensitive, large-scale maps of the CO J=1-0 emission of the L1448 dark cloud. These maps were acquired using the On-The-Fly capability of the NRAO 12-meter telescope. CO outflow activity is seen in L1448 on parsec-scales for the…

Astrophysics · Physics 2009-10-31 G. A. Wolf-Chase , M. Barsony , J. O'Linger