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Related papers: A Pulsed, Precessing Jet in Cepheus A

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We compile position and inclination angles for tilted ring fits to the warped dusty and gaseous disk spanning radius 1.8 to 6500 pc from recent observations. For radii exterior to a kpc, tilted ring orientations lie on an arc on a polar…

Astrophysics of Galaxies · Physics 2015-05-14 Alice C. Quillen , Nadine Neumayer , Tom Oosterloo , Daniel Espada

We report the discovery of an extremely curved jet in the radio-loud quasar PKS2136+141. Multi-frequency Very Long Baseline Array (VLBA) images show a bending jet making a turn-around of 210 degrees in the plane of the sky, which is, to our…

We present the first detection of the H40a, H34a and H31a radio recombination lines (RRLs) at millimeter wavelengths toward the high-velocity, ionized jet in the Cepheus A HW2 star forming region. From our single-dish and interferometric…

Solar and Stellar Astrophysics · Physics 2015-05-27 Izaskun Jimenez-Serra , Jesus Martin-Pintado , Alejandro Baez-Rubio , Nimesh Patel , Clemens Thum

Recent Hubble Space Telescope (HST) observations of the extragalactic radio source Centaurus A (Cen A) display a young stellar population around the southwest tip of the inner filament 8.5 kpc from the Cen A galactic center, with ages in…

Astrophysics of Galaxies · Physics 2017-02-08 Carl L. Gardner , Jeremiah R. Jones , Evan Scannapieco , Rogier A. Windhorst

We observed molecular hydrogen around a sample of pre-main sequence stars in order to better characterize their gaseous CS environments. We analyzed the FUSE (Far Ultraviolet Spectroscopic Explorer) spectra of a sample of Herbig Ae/Be stars…

A few years ago, we investigated MYSO G29.862-0.0044 (YSO-G29), an intriguing star-forming region at a distance of 6.2 kpc. Although the typical disc-jet scenario was proposed to explain the observations, it remained far from conclusive.…

Astrophysics of Galaxies · Physics 2025-10-01 S. Paron , N. C. Martinez , M. E. Ortega , D. Mast , A. Petriella , L. Supán , C. Fariña

We present near infrared images in H2 at 2.12um of the HH 7/11 outflow and its driving source SVS 13 taken with HST NICMOS 2 camera, as well as archival Ha and [SII] optical images obtained with the WFPC2 camera. The NICMOS high angular…

Astrophysics · Physics 2009-11-07 A. Noriega-Crespo , A. Cotera , E. Young , H. Chen

We present neutral hydrogen, ultraviolet, optical and near-infrared imaging, and optical spectroscopy, of Minkowski's Object (MO), a star forming peculiar galaxy near NGC 541. The observations strengthen evidence that star formation in MO…

We present hydrodynamical calculations carried out with the 3D yguazu-a code of a precessing jet model, which interacts with a plane parallel wind. This scenario describes an extragalactic jet, in which the jet source is in motion with…

We present new, sensitive, near-infrared images of the Class I protostar, Elias 29, in the Ophiuchus cloud core. To explore the relationship between the infall envelope and the outflow, narrowband H2 1-0 S(1), Br-gamma, and narrowband…

The central problem in forming a star is the angular momentum in the circumstellar disk which prevents material from falling into the central stellar core. An attractive solution to the "angular momentum problem" appears to be the…

Astrophysics of Galaxies · Physics 2017-06-21 Chin-Fei Lee , Paul. T. P Ho , Zhi-Yun Li , Naomi Hirano , Qizhou Zhang , Hsien Shang

Jet precession is sometimes invoked to explain asymmetries in radio galaxy (RG) jets and "X/S/Z-shape" radio galaxies, caused by the presence of a binary black hole companion to the source active galactic nucleus (AGN) or by accretion…

High Energy Astrophysical Phenomena · Physics 2023-05-08 Chris Nolting , Jay Ball , Tri M. Nguyen

Observations of the atomic and molecular line emission associated with jets and outflows emitted by young stellar objects can be used to trace the various evolutionary stages they pass through as they evolve to become main sequence stars.…

Solar and Stellar Astrophysics · Physics 2015-06-05 L. Podio , I. Kamp , D. Flower , C. Howard , G. Sandell , A. Mora , G. Aresu , S. Brittain , W. F. R. Dent , C. Pinte , G. J. White

The first map of interstellar acetylene (C2H2) has been obtained with the infrared spectrograph onboard the Spitzer Space Telescope. A spectral line map of the $\nu_5$ vibration-rotation band at 13.7 microns carried out toward the…

Astrophysics · Physics 2009-11-13 P. Sonnentrucker , E. González-Alfonso , D. A. Neufeld

The circumstellar medium around massive stars is strongly impacted by stellar winds, radiation, and explosions. We use numerical simulations of these interactions to constrain the current properties and evolutionary history of various stars…

Centaurus A is one of the closest radio-galaxies to Earth. Its proximity allowed us to extensively study its active galactic nucleus but the core emission mechanism remains elusive because of local strong dust and gas obscuration. The…

Protostars interact with their surroundings through jets and winds impacting on the envelope and creating shocks, but the nature of these shocks is still poorly understood. Our aim is to survey far-infrared molecular line emission from a…

Near-IR atomic and molecular transitions are powerful tools to trace the warm and hot gas in the circumstellar environment of young stars. Ro-vibrational transitions of H2 and H2O, and overtone transitions of CO at 2 micron centered at the…

Instrumentation and Methods for Astrophysics · Physics 2013-10-09 A. Carmona , J. Bouvier , X. Delfosse

We present a Spitzer Infrared Spectrograph (IRS) map of H2 emission from the nearby galaxy NGC 4258 (Messier 106). The H2 emission comes from 9.4E6 Msun of warm molecular hydrogen heated to 240-1040 K in the inner anomalous arms, a…

Astrophysics of Galaxies · Physics 2015-06-19 Patrick M. Ogle , Lauranne Lanz , Philip N. Appleton

We present the results of millimetre (33 and 35 GHz) and centimetre (2.1, 5.5 and 9.0 GHz) wavelength observations of the neutron star X-ray binary Circinus X-1, using the Australia Telescope Compact Array. We have used advanced calibration…

High Energy Astrophysical Phenomena · Physics 2019-01-16 M. Coriat , R. Fender , C. Tasse , O. Smirnov , A. K. Tzioumis , J. W. Broderick
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