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相关论文: HH 46/47: Also a parsec scale flow

200 篇论文

We report here the discovery of a 30"-chain of embedded Herbig-Haro (HH) objects in the rho Ophiuchi dark cloud. These HH objects were first detected during a deep K_S-band observation (completeness magnitude for point source~19) made with…

天体物理学 · 物理学 2009-11-07 Nicolas Grosso , Joao Alves , Ralph Neuhaeuser , Thierry Montmerle

We discuss wide-field near-IR imaging of the NGC1333, L1448, L1455 and B1 star forming regions in Perseus. The observations have been extracted from a much larger narrow-band imaging survey of the Taurus-Auriga-Perseus complex. These H2…

天体物理学 · 物理学 2009-06-23 C. J. Davis , P. Scholz , P. Lucas , M. D. Smith , A. Adamson

Massive outflows of neutral atomic hydrogen (HI) have been observed in absorption in a number of radio galaxies and are considered a signature of AGN feedback. These outflows on kpc-scales have not been investigated in great detail as they…

星系天体物理 · 物理学 2021-03-17 R. Schulz , R. Morganti , K. Nyland , Z. Paragi , E. K. Mahony , T. Oosterloo

HH 666 is an externally irradiated protostellar outflow in the Carina Nebula for which we present new near-IR [Fe II] spectra obtained with the FIRE spectrograph at Magellan Observatory. Earlier H{\alpha} and near-IR [Fe II] imaging…

太阳与恒星天体物理 · 物理学 2015-06-24 Megan Reiter , Nathan Smith , Megan M. Kiminki , John Bally

We have used the Hubble Space Telescope to acquire new broad-band and narrow-band images of the optical line emission and red continuum associated with the HH 7-11 stellar jet in the NGC 1333 star formation region. Combining the new…

太阳与恒星天体物理 · 物理学 2019-05-29 P. Hartigan , R. Holcomb , A. Frank

We have identified a new externally irradiated Herbig-Haro (HH) jet, HH 1158, within ~2 pc of the massive OB type stars in the sigma Orionis cluster. At an Lbol ~ 0.1 Lsun, HH 1158 is the lowest luminosity irradiated HH jet identified to…

太阳与恒星天体物理 · 物理学 2015-12-23 B. Riaz , E. T. Whelan

Hubble Space Telescope images obtained in 2018 are combined with archival HST data taken in 1995 to detect changes and measure proper motions in the HH 80/81 shock complex which is powered by the fastest known jet driven by a forming star,…

星系天体物理 · 物理学 2023-08-29 John Bally , Bo Reipurth

We have surveyed the inner 5' of the Orion Nebula by means of Halpha and [NII] Fabry-Perot imaging spectroscopy to present a kinematical study of the Herbig-Haro objects in the nebula. The objects studied in this work are HH 202, 203, 204,…

天体物理学 · 物理学 2009-11-06 Margarita Rosado , Eduardo de la Fuente , Lorena Arias , Alejandro Raga , Ettiane Le Coarer

We report the results of a spatially compete, high-sensitivity survey for Herbig-Haro (HH) outflows in the Western and Eastern Circinus molecular clouds. We have detected 28 new HH objects in Circinus West, doubling the number known in this…

星系天体物理 · 物理学 2025-03-20 T. A. Rector , L. Prato , R. Kerr , E. Papraniku , K. Fisk

High-resolution infrared spectroscopy in the 2.3-4.6 micron region is reported for the peculiar A supergiant, single-lined spectroscopic binary HR 4049. Lines from the CO fundamental and first overtone, OH fundamental, and several H2O…

天体物理学 · 物理学 2009-06-23 Kenneth H. Hinkle , Sean D. Brittain , David L. Lambert

We analyze the H2 emission observed in the HH46 Class I system as part of PROJECT-J (Protostellar Jets Cradle Tested with JWST), to investigate the origin and excitation of the warm molecular outflow. We used NIRSpec and MIRI spectral maps…

Stretching a length reaching 10 pc projected in the plane of sky, the radio jet associated with Herbig-Haro objects 80 and 81 (HH 80-81) is known as the largest and best collimated protostellar jet in our Galaxy. The nature of the molecular…

星系天体物理 · 物理学 2019-05-01 Keping Qiu , Friedrich Wyrowski , Karl Menten , Qizhou Zhang , Rolf Guesten

The overall properties of the Herbig-Haro objects such as centerline velocity, transversal profile of velocity, flow of mass and energy are explained adopting two models for the turbulent jet. The complex shapes of the Herbig-Haro objects,…

星系天体物理 · 物理学 2011-09-20 Lorenzo Zaninetti

We present results of the narrow-band Halpha and [SII] imaging survey of Mon R1 association, performed with the 1 m Schmidt telescope of the Byurakan Observatory. Our observations covered one degree field near the center of the association.…

太阳与恒星天体物理 · 物理学 2020-12-02 T. A. Movsessian , T. Yu. Magakian , S. N. Dodonov

We present infrared echelle spectroscopy of three Herbig-Haro (HH) driving sources (SVS 13, B5-IRS 1 and HH 34 IRS) using Subaru-IRCS. The large diameter of the telescope and wide spectral coverage of the spectrograph allowed us to detect…

天体物理学 · 物理学 2009-11-13 M. Takami , A. Chrysostomou , T. P. Ray , C. J. Davis , W. R. F. Dent , J. Bailey , M. Tamura , H. Terada , T. S. Pyo

This paper reports on the detection of a likely explosive outflow in the high-mass star-forming complex G34.26+0.15, adding to the small number (six) of explosive outflows detected so far. ALMA CO(2-1) and SiO(5-4) archival observations…

太阳与恒星天体物理 · 物理学 2025-04-23 Namitha Issac , Xing Lu , Tie Liu , Luis A Zapata , Hong-Li Liu , Anandmayee Tej , Yan-Kun Zhang , Wenyu Jiao , Suinan Zhang

We present a new analysis of the physical conditions in three Herbig-Haro complexes (HH 54, HH 212, and the L 1157 protostellar jet) using archival data from the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. As described in…

太阳与恒星天体物理 · 物理学 2015-05-30 Michihiro Takami , Jennifer L. Karr , Brunella Nisini , Thomas P. Ray

A number of extragalactic radio sources which exhibit symmetric jets on parsec scales have now been found to have neutral hydrogen absorption at or near the systemic velocities of their host galaxies. Understanding the spatial distribution…

天体物理学 · 物理学 2009-11-06 A. B. Peck , G. B. Taylor

We present ALMA Cycle 1 observations of the HH46/47 molecular outflow using combined 12m array and ACA observations. The improved angular resolution and sensitivity of our multi-line maps reveal structures that help us study the entrainment…

The giant Herbig-Haro object 222 extends over $\sim$6$'$ in the plane of the sky, with a bow shock morphology. The identification of its exciting source has remained uncertain over the years. A non-thermal radio source located at the core…

太阳与恒星天体物理 · 物理学 2016-10-12 L. F. Rodriguez , J. O. Yam , C. Carrasco-Gonzalez , G. Anglada , A. Trejo