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We present new, high dynamic range VLA images of the inner jet of the closest radio galaxy, Centaurus A. Over a ten-year baseline we detect apparent sub-luminal motions (v ~ 0.5c) in the jet on scales of hundreds of pc. The inferred speeds…

天体物理学 · 物理学 2008-11-26 M. J. Hardcastle , D. M. Worrall , R. P. Kraft , W. R. Forman , C. Jones , S. S. Murray

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

Aims: We employ archival Spitzer slit-scan observations of the HH211 outflow in order to investigate its warm gas content, assess the jet mass flux in the form of H2 and probe for the existence of an embedded atomic jet. Methods: Detected…

星系天体物理 · 物理学 2015-05-19 O. Dionatos , B. Nisini , S. Cabrit , L. Kristensen , G. Pineau des Forets

We report detailed studies of the X-ray emission from the kpc scale jet in the nearest active galaxy, Cen A. 41 compact sources were found within the jet, 13 of which were newly identified. We construct the luminosity function for the…

We present H-alpha and [O III] (5007 Angstroms) images of the nebula powered by the jet of the black hole candidate and microquasar Cygnus X-1, observed with the 2.5m Isaac Newton Telescope (INT). The ring-like structure is luminous in [O…

天体物理学 · 物理学 2008-11-26 D. M. Russell , R. P. Fender , E. Gallo , C. R. Kaiser

Aims: Previous observations of the young massive star formation region IRAS 19410+2336 have revealed strong outflow activity with several interacting outflows. We aim to get a better understanding of the outflow activity in this region by…

星系天体物理 · 物理学 2016-04-13 Felix Widmann , Henrik Beuther , Peter Schilke , Thomas Stanke

Sensitive 5-38 um Spitzer Space Telescope (SST) and ground based 3-5 um spectra of the embedded low mass protostars B5 IRS1 and HH46 IRS show deep ice absorption bands superposed on steeply rising mid-infrared continua. The ices likely…

We present initial results from JWST NIRSpec integral field unit observations of the nearby Supernova (SN) 1987A. The observations provide the first spatially-resolved spectroscopy of the ejecta and equatorial ring (ER) over the 1-5 \mu m…

We present observations of the high-mass star-forming region S255IR, which harbors the $\sim$20 M$_\odot$ protostar NIRS3, where a disk-mediated accretion burst was recorded several years ago, with the angular resolution of $\sim$15 mas,…

星系天体物理 · 物理学 2024-12-18 I. I. Zinchenko , S. -Y. Liu , Y. -N. Su

We present high-resolution VLT/UVES spectroscopy and a detailed analysis of the unique Broad Absorption-Line system towards the quasar SDSS J165252.67+265001.96. This system exhibits low-ionization metal absorption lines from the ground…

星系天体物理 · 物理学 2023-07-28 Balashev S. A. , Ledoux C. , Noterdaeme P. , Boissé P. , Krogager J. K. , López S. , Telikova K. N

The origin of X-ray emission from the resolved kiloparsec-scale jets and hotspots of many active galactic nuclei (AGN) remains uncertain, particularly where the X-ray emission is separate from the radio-optical synchrotron component.…

高能天体物理现象 · 物理学 2024-06-06 Aamil Shaik , Eileen T. Meyer , Karthik Reddy , Sibasish Laha , Markos Georganopoulos

We report near infrared (NIR) spectroscopic observations of twelve ``Branch-normal'' Type Ia supernovae (SNe Ia) which cover the wavelength region from 0.8-2.5 microns. Our sample more than doubles the number of SNe Ia with published NIR…

天体物理学 · 物理学 2009-11-10 G. H. Marion , P. Höflich , W. D. Vacca , J. C. Wheeler

We present new observations of the CB130 region, composed of three separate cores. Using the \textit{Spitzer Space Telescope} we detected a Class 0 and a Class II object in one of these, CB130-1. The observed photometric data from…

High resolution observations of Young Stellar Object (YSO) jets show them to be composed of many small-scale knots or clumps. In this paper we report results of 3-D numerical simulations designed to study how such clumps interact and create…

高能天体物理现象 · 物理学 2017-03-22 E. C. Hansen , A. Frank , P. Hartigan , S. V. Lebedev

JWST/MIRI has sharpened our infrared eyes toward the star formation process. This paper presents the first mid-infrared detection of gaseous SO$_2$ emission in an embedded low-mass protostellar system. MIRI-MRS observations of the low-mass…

We present an analysis of the kinematics and physical properties of the Class I driven jet HH46-47 based on IR medium and low resolution spectroscopy obtained with ISAAC on VLT. Our aim is to study the gas physics as a function of the…

太阳与恒星天体物理 · 物理学 2015-05-14 Rebeca Garcia Lopez , Brunella Nisini , Jochen Eisloeffel , Teresa Giannini , Francesca Bacciotti , Linda Podio

Space-based mid-IR spectroscopy provides tracers of warm gas in star-forming regions that are inaccessible from the ground. Past mid-IR spectra of bright high-mass protostars in the hot-core phase typically showed strong absorption features…

We present evidence for an X-ray jet in the T Tau star DG Tau A based on Chandra ACIS data. DG Tau A, a jet-driving classical T Tau star with a flat infrared spectrum, reveals an unusual X-ray spectrum that requires two thermal components…

天体物理学 · 物理学 2009-11-11 M. Guedel , S. L. Skinner , K. R. Briggs , M. Audard , K. Arzner , A. Telleschi

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

Aims. To increase the observational samples of star formation around expanding Hii regions, we analyzed the interstellar medium and star formation around N22. Methods. We used data extracted from the seven large-scale surveys from infrared…

星系天体物理 · 物理学 2012-06-14 W. G. Ji , J. J. Zhou , J. Esimbek , Y. F. Wu , G. Wu , X. D. Tang