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相关论文: [Fe II] 1.64 um Features of Jets and Outflows from…

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We present observations of ionized gas outflows in eleven z$ =1.39-2.59$ radio-loud quasar host galaxies. Data was taken with the integral field spectrograph (IFS) OSIRIS and the adaptive optics system at the W.M. Keck Observatory targeting…

We present the first detection of a jet in the far-IR [O I] lines from an intermediate mass protostar. We have carried out a Herschel/PACS spectral mapping study in the [O I] lines of OMC-2 FIR 3 and FIR 4, two of the most luminous…

We present the results of Keck Telescope laser adaptive optics integral field spectroscopy with OSIRIS of the innermost regions of the NGC 1333 SVS 13 outflow that forms the system of Herbig-Haro objects 7-11. We find a bright 0.2 arc sec…

太阳与恒星天体物理 · 物理学 2015-06-22 Klaus W. Hodapp , Rolf Chini

While there are many parsec-scale Herbig-Haro (HH) outflows known to be driven by low-mass young stars, few are associated with their intermediate mass counterparts. Here we present the discovery of five such bipolar outflows. Of these,…

天体物理学 · 物理学 2009-11-10 Fiona McGroarty , Tom Ray , John Bally

We have identified ionized outflows in the narrow line region of all but one SDSS type 2 quasars (QSO2) at z<~0.1 (20/21, detection rate 95%), implying that this is a ubiquitous phenomenon in this object class also at the lowest z. The…

星系天体物理 · 物理学 2015-06-19 M. Villar Martin , B. Emonts , A. Humphrey , A. Cabrera Lavers , L. Binette

We present results from a coordinated, multi-epoch near-infrared and centimeter radio survey of young stellar objects (YSOs) in the Coronet, aimed at probing the connection between mass accretion and ionised mass loss. Using VLT-KMOS, we…

We present a detailed study of the kinematics of 19 QSO2s in the range 0.3<z<0.41 and [OIII] luminosities $L_{[OIII]} > 10^{8.5}$L$_{\odot}$. We aim at advancing our understanding of the AGN feedback phenomenon by correlating outflow…

We present Spitzer IRAC images that indicate the presence of cavities cut into the dense outer envelope surrounding very young pre-main sequence stars. These young stellar objects (YSOs) characterized by an outflow represent the earliest…

天体物理学 · 物理学 2007-11-28 Jonathan P. Seale , Leslie W. Looney

We present new infrared data from a survey for embedded protostellar jets in the Orion A cloud. This survey makes use of the S(1) v = 1-0 line of molecular hydrogen at lambda = 2.12 mum to search for infrared jets deep inside the cloud and…

天体物理学 · 物理学 2007-05-23 Thomas Stanke , Mark J. McCaughrean , Hans Zinnecker

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…

天体物理学 · 物理学 2009-10-31 John Bally , Bo Reipurth

We present the spectral and spatial evolution of H$_2$O masers associated with the water fountain source IRAS 18043$-$2116 found in the observations with the Nobeyama 45 m telescope and the Australia Telescope Compact Array. We have found…

太阳与恒星天体物理 · 物理学 2023-05-10 L. Uscanga , H. Imai , J. F. Gómez , D. Tafoya , G. Orosz , T. P. McCarthy , Y. Hamae , K. Amada

Over the past few years, chemical studies have revealed multiple structures in the vicinity of young stellar objects (YSOs). It has become evident that specific physical conditions are associated with the emission of particular molecular…

太阳与恒星天体物理 · 物理学 2024-07-03 M. Tanious , R. Le Gal , R. Neri , A. Faure , A. Gupta , C. J. Law , J. Huang , N. Cuello , J. P. Williams , F. Ménard

Cygnus OB2 is the most massive association within 2kpc from the Sun, hosting hundreds of massive stars, thousands of young low mass members, and some sights of active star formation in the surrounding cloud. Recently, 10 photoevaporating…

太阳与恒星天体物理 · 物理学 2015-06-22 M. G. Guarcello , J. J. Drake , N. J. Wright , D. Garcìa-Alvarez , K. E. Kraemer

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 investigate the emissivity properties of the main near-IR transitions of the Fe+ ion in the conditions prevailing in the inner regions of jets from young stars, based on a simplified 16-level atom model. We present new diagnostic…

天体物理学 · 物理学 2009-11-10 N. Pesenti , C. Dougados , S. Cabrit , D. O'Brien , P. Garcia , J. Ferreira

Theoretical models suggest that massive stars form via disk-mediated accretion, with bipolar outflows playing a fundamental role. A recent study toward massive molecular outflows has revealed a decrease of the SiO line intensity as the…

We present the results of an outflow and infall survey towards a distance limited sample of 31 massive star forming regions drawn from the RMS survey. The presence of young, active outflows is identified from SiO (8-7) emission and the…

星系天体物理 · 物理学 2018-04-04 Nichol Cunningham , Stuart Lumsden , Toby Moore , Luke Maud , Ignacio. Mendigutia

Aims: We want to study the physical properties of the ionized jet emission in the vicinity of an O-type young stellar object (YSO), and estimate how efficient is the transfer of energy and momentum from small- to large-scale outflows.…

星系天体物理 · 物理学 2016-12-07 A. Sanna , L. Moscadelli , R. Cesaroni , A. Caratti o Garatti , C. Goddi , C. Carrasco-González

Context. The Gum 31 bubble containing the stellar cluster NGC 3324 is a poorly-studied young region close to the Carina Nebula. Aims. We are aiming to characterise the young stellar and protostellar population in and around Gum 31 and to…