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We present a high-resolution, near-IR spectroscopic study of multiple outflows in the LkH$\alpha$ 234 star formation region using the Immersion GRating INfrared Spectrometer (IGRINS). Spectral mapping over the blueshifted emission of HH 167…

To reveal the origins of diffuse H-alpha emissions observed around the Herbig star MWC 1080, we have performed a high-resolution near-infrared (NIR) spectroscopic observation using the Immersion GRating INfrared Spectrograph (IGRINS). In…

星系天体物理 · 物理学 2021-06-30 Il-Joong Kim , Heeyoung Oh , Woong-Seob Jeong , Kwang-Il Seon , Tae-Soo Pyo , Jae-Joon Lee

We report on spectro-imaging observations of the Herbig-Haro 2 outflow with the ISOCAM camera onboard the Infrared Space Observatory (ISO). The [Ne II}] 12.81 microns and [Ne III]15.55 microns lines are detected only towards the jet working…

天体物理学 · 物理学 2009-11-07 B. Lefloch , J. Cernicharo , S. Cabrit , A. Noriega-Crespo , A. Moro-Martin , D. Cesarsky

At present there are many studies concerning jets towards low-mass young stellar objects, while equivalent studies towards massive or intermediate-mass young stellar objects are scarce. In a previous study, we found highly misaligned…

星系天体物理 · 物理学 2016-10-05 S. Paron , C. Fariña , M. E. Ortega

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

Abridged. The bright-rimmed cloud IC1396N hosts CO, H$_2$, and Herbig-Haro outflows powered by millimetre compact sources. We aim to characterise the kinematics and physical conditions of the H$_2$ emission features spread over IC1396N,…

星系天体物理 · 物理学 2022-08-10 Fabrizio Massi , Rosario López , Maria T. Beltrán , Robert Estalella , Josep M. Girart

We present the detection, performed with the Westerbork Synthesis Radio Telescope (WSRT) and the Karl Jansky Very Large Array (VLA), of a fast HI 21-cm outflow in the ultra-luminous infrared galaxy Mrk 231. The outflow is observed as…

星系天体物理 · 物理学 2016-09-07 Raffaella Morganti , Sylvain Veilleux , Tom Oosterloo , Stacy H. Teng , David Rupke

We present high spatial resolution optical integral field spectroscopy of a collimated Herbig-Haro jet viewed nearly edge-on. Maps of the line emission, velocity centroid, and velocity dispersion were generated for the H$\alpha$ and [S II]…

天体物理学 · 物理学 2008-11-26 Tracy L. Beck , A. Riera , A. C. Raga , Bo Reipurth

We have observed optical (Halpha and [SII]) and near-IR (S(1) line of H2) deep fields and taken optical spectra using the 2.56m NOT, as well as a near-UV deep field (U band) using the 3.58m NTT. In addition we present new SPITZER (IRAC and…

天体物理学 · 物理学 2009-11-13 M. Gålfalk , G. Olofsson

The dark cloud Lynds 723 (L723) is a low-mass star-forming region where one of the few known cases of a quadrupolar CO outflow has been reported. Two recent works have found that the radio continuum source VLA 2, towards the centre of the…

星系天体物理 · 物理学 2015-05-19 R. Lopez , J. A. Acosta-Pulido , G. Gomez , R. Estalella , C. Carrasco-Gonzalez

Jets and outflows are associated with young stellar objects across the stellar mass spectrum, from brown dwarf protostars to massive, Ae/Be stars. Frequently, the jet morphology is spatially discontinuous because of the temporal variability…

太阳与恒星天体物理 · 物理学 2021-04-14 Rosario López , Angels Riera , Robert Estalella , Gabriel Gómez

We present high resolution images of NGC 2071-IR in the $J$, $H$, and $K$ bands and in the emission at 2.12 $\mu$m of the v=$1-0$ $S$(1) line of molecular hydrogen. We also present moderate resolution K-band spectra of two young stellar…

星系天体物理 · 物理学 2021-03-12 D. M. Walther , T. R. Geballe

We present here an extensive analysis of the protostellar jet driven by IRAS 20126+4104, deriving the kinematical, dynamical, and physical conditions of the H2 gas along the flow. The jet has been investigated by means of near-IR H2 and…

天体物理学 · 物理学 2015-05-13 A. Caratti o Garatti , D. Froebrich , J. Eisloeffel , T. Giannini , B. Nisini

We report here on the first proper motion measurements of molecular hydrogen emission features in the Herbig-Haro 46/47 outflow. Assuming a distance of 350 pc to this flow, the inferred tangential velocities range from a few tens to almost…

Long slit spectra of the molecular outflow Herbig-Haro (HH) 46/47 has been taken in the J and K near-infrared bands. The observed H2 line emission confirms the existence of a bright and extended redshifted counter-jet outflow southwest of…

天体物理学 · 物理学 2009-10-31 Amadeu Fernandes

Massive stars form deeply embedded in their parental clouds, making it challenging to directly observe these stars and their immediate environments. It is known that accretion and ejection processes are intrinsically related, thus observing…

太阳与恒星天体物理 · 物理学 2022-07-20 A. R. Costa Silva , R. Fedriani , J. C. Tan , A. Caratti o Garatti , S. Ramsay , V. Rosero , G. Cosentino , P. Gorai , S. Leurini

With the Spitzer-IRS we have obtained the first mid-IR spectroscopy of NGC 7129, in the unusually strong outflow and in a ridge of H_2 emission near the Herbig Be star LkHalpha-234. The UV radiation field strength is estimated from PAH band…

天体物理学 · 物理学 2009-11-10 P. W. Morris , A. Noriega-Crespo , F. R. Marleau , H. I. Teplitz , K. I. Uchida , L. Armus

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

To trace the accretion and outflow processes around YSOs, diagnostic spectral lines such as the BrG 2.166 micron line are widely used, although due to a lack of spatial resolution, the origin of the line emission is still unclear. Employing…

We present near infrared (IR) spectra (0.98--2.5 mu m) from the group of Herbig-Haro (HH) objects comprising HH99: a series of knots forming a bow, HH99B, and a separate knot, HH99A. Observations of H2, [Fe II] and [C I] are used to…

天体物理学 · 物理学 2009-11-10 C. McCoey , T. Giannini , D. R. Flower , A. Caratti o Garatti
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