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Related papers: HH 46/47: Also a parsec scale flow

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We present wide-field, high-resolution imaging observations in 12CO 3-2 and H2 1-0 S(1) towards a ~1 square degree region of NGC2264. We identify 46 H2 emission objects, of which 35 are new discoveries. We characterize several cores as…

Astrophysics of Galaxies · Physics 2015-06-04 J. V. Buckle , J. S. Richer , C. J. Davis

We present a parsec-scale molecular hydrogen (H$_2$ 1-0 S(1) at 2.12~\micron) outflow discovered from the UKIRT Widefield Infrared Survey for H$_2$. The outflow is located in the infrared dark cloud core MSXDC G053.11+00.05 MM1 at 1.7 kpc…

Astrophysics of Galaxies · Physics 2018-08-15 Hyun-Jeong Kim , Bon-Chul Koo , Tae-Soo Pyo , Christopher J. Davis

We present the results of high-resolution near-IR spectroscopy toward the multiple outflows around the Herbig Be star Lk{\Ha} 234 using the Immersion Grating Infrared Spectrograph (IGRINS). Previous studies indicate that the region around…

We report the discovery of a dozen Herbig-Haro jets illuminated by the Lyman continuum and/or softer far-ultraviolet radiation fields of nearby high mass stars. Five irradiated outflows lie in the outer parts of the Orion Nebula and seven…

Astrophysics · Physics 2009-10-31 John Bally , Bo Reipurth

Spectral monitoring of the yellow hypergiant $\rho$ Cas with the by 6-m telescope of the Special Astrophysical Observatory with a spectral resolution of R$\ge$60000 has led to the detection of new features in the kinematic state of its…

Solar and Stellar Astrophysics · Physics 2018-08-29 V. G. Klochkova , V. E. Panchuk , N. S. Tavolzhanskaya

Previous studies of young stellar objects (YSOs) have uncovered a number of associated parsec-scale optical outflows, the majority of which are driven by low-mass, embedded Class I sources. Here we examine more evolved Classical T Tauri…

Astrophysics · Physics 2009-11-10 F. McGroarty , T. P. Ray

Knotty structures of Herbig-Haro jets are common phenomena, and knowing the origin of these structures is essential for understanding the processes of jet formation. Basically, there are two theoretical approaches: different types of…

Solar and Stellar Astrophysics · Physics 2015-06-04 T. A. Movsessian , T. Yu. Magakian , A. V. Moiseev

The two spectrometers on board the Infrared Space Observatory were used to observe the Herbig-Haro objects HH 80, 81 and 80N, as well as their candidate exciting source IRAS 18162-2048. The fine structure lines of [OI]63um, [OI]145um and…

Astrophysics · Physics 2009-10-31 Sergio Molinari , Alberto Noriega-Crespo , Luigi Spinoglio

SN 2014C was originally classified as a Type Ib supernova, but at phase {\phi} = 127 d post-explosion strong H{\alpha} emission was observed. SN 2014C has since been observed in radio, infrared, optical and X-ray bands. Here we present new…

Multiple optical outflows are known to exist in the vicinity of the active star formation region called Orion-South (Orion-S). We have mapped the velocity of low ionization features in the brightest part of the Orion Nebula, including…

We aimed to map the jets and outflows from the Serpens South star forming region and find an empirical relationship between the magnetic field and outflow orientation. Near-infrared H2 v=1-0 S(1) 2.122{\mu}m -line imaging of the \sim…

Solar and Stellar Astrophysics · Physics 2015-06-04 G. D. C. Teixeira , M. S. N. Kumar , R. Bachiller , J. M. C. Grave

We present high resolution images of the radio source 3C 84 at 43 GHz, from 121 observations conducted by the BEAM-ME monitoring program between 2010 and 2023. Imaging was performed using the recent forward modeling imaging method…

High Energy Astrophysical Phenomena · Physics 2025-04-02 M. Foschi , J. L. Gómez , A. Fuentes , I. Cho , A. P. Marscher , S. Jorstad

We have obtained maps of the large scale outflow associated with the UCHII regionG5.89-0.39 in CO and 13CO (J=3-2), SiO (J=8-7,J=5-4), SO2 (13(2,12)-13(1,13)) and H13CO+(J=4-3). From these maps we have been able to determine the mass (3.3…

Astrophysics · Physics 2008-11-26 P. D. Klaassen , R. Plume , R. Ouyed , A. M. von Benda-Beckmann , J. Di Francesco

Aims. We present a detailed study of the infrared line emission (1-200 micron) in the Herbig-Haro object HH54. Our database comprises: high- (R~9000) and low- (R~600) resolution spectroscopic data in the near-infrared band (1-2.5 micron);…

We present the results of Very Large Array NH$_{3}$ $(J,K)=(1,1)$ and $(2,2)$ observations of the HH 111/HH 121 protostellar system. HH 111, with a spectacular collimated optical jet, is one of the most well-known Herbig-Haro objects. We…

We present the results of deep, high angular resolution Very Large Array (VLA) surveys for radio continuum emission towards a sample of 14 GLIMPSE Extended Green Objects (EGOs). Identified as massive young stellar object (MYSO) outflow…

Solar and Stellar Astrophysics · Physics 2015-05-30 C. J. Cyganowski , C. L. Brogan , T. R. Hunter , E. Churchwell

We present five epochs of VLBI water maser observations around the massive protostar Cepheus A HW2 with 0.4 mas (0.3 AU) resolution. The main goal of these observations was to follow the evolution of the remarkable water maser…

Solar and Stellar Astrophysics · Physics 2015-05-19 J. M. Torrelles , N. A. Patel , S. Curiel , R. Estalella , J. F. Gomez , L. F. Rodriguez , J. Canto , G. Anglada , W. Vlemmings , G. Garay , A. Raga , P. T. P. Ho

We have obtained Hubble Space Telescope STIS and NICMOS, and Gemini/GPI scattered light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling Kuiper Belt in radial extent (FWHM: ${\sim}$25 au, centered…

New, high-sensitivity interferometric CO J=2-1 observations of the HH 7-11 outflow show that despite previous doubts, this system is powered by the Class I source SVS 13. The molecular outflow from SVS 13 is formed by a shell with a large…

Astrophysics · Physics 2007-05-23 R. Bachiller , F. Gueth , S. Guilloteau , M. Tafalla , A. Dutrey

Jets and outflows are the first signposts of stellar birth. Emission in the H2 1-0S(1) line at 2.122 micron is a powerful tracer of shock excitation in these objects. Here we present the analysis of 2.0 x 0.8 square degrees data from the UK…

Astrophysics of Galaxies · Physics 2018-06-06 Manash R. Samal , Wen-Ping Chen , Michihiro Takami , Jessy Jose , Dirk Froebrich
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