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Related papers: Herbig-Haro objects around CG 30

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The physical parameters of Herbig-Haro jets are usually determined from emission line ratios, obtained from spectroscopy or narrow band imaging, assuming that the emitting region is homogeneous along the line of sight. Under the more…

Solar and Stellar Astrophysics · Physics 2019-08-19 Fabio De Colle , Carlos del Burgo , Alejandro Raga

We present a wide-field survey of the young open cluster IC348 for molecular H2 outflows. Outflow activity is only found at its south-western limit, where a new subcluster of embedded sources is in an early phase of its formation. If the…

Astrophysics · Physics 2009-11-07 J. Eislöffel , D. Froebrich , T. Stanke , M. J. McCaughrean

M31 hosts a rich population of outer halo ($R_{\rm{proj}} > 25$ kpc) globular clusters (GCs), many of which show strong evidence for spatial and/or kinematical associations with large-scale tidal debris features. We present deep Hubble…

Two new Herbig-Haro flows were found in a study of the isolated Dobashi 5006 dark cloud (l$= 216^\circ.7$, b= $-$13$^\circ.9$): one certain (HH 1179) and one presumable, associated with the infrared sources 2MASS 06082284$-$0936139 and…

Solar and Stellar Astrophysics · Physics 2023-04-26 T. A. Movsessian , T. Yu. Magakian , A. S. Rastorguev , H. R. Andreasyan

Long-slit observations of the blue compact galaxy Haro 2 have been performed to detect the Halpha emission originating in the partially ionized wind outflowing at 200 km/s, that had been previously detected with the Hubble Space Telescope.…

Astrophysics · Physics 2007-05-23 F. Legrand , D. Kunth , J. M. Mas-Hesse , J. Lequeux

High quality 4500-6800 A spectropolarimetric observations of the Circinus galaxy are reported. These show polarized and relatively broad (FWHM~3300 km/s) Halpha (as well as marginal Hbeta) arising from a <3" (<60 pc) region centered on the…

Astrophysics · Physics 2007-05-23 E. Oliva , A. Marconi , A. Cimatti , S. di Serego Alighieri

We present observations of continuum emission in the MIR to mm wavelength range, complemented with ammonia observations, of the dense core ahead of the radio Herbig Haro object HH 80N, found in the GGD 27 region. The continuum emission in…

We have completed a survey of 30 Virgo cluster galaxies in the Halpha emission-line using Fabry-Perot interferometry. The goal of the survey is to obtain a high angular resolution sample of velocity fields of spirals and to study the…

A long slit spectrum from the barred galaxy NGC 1415 has been obtained with the 2.1m Guillermo Haro telescope in Cananea, Mexico at position angle 155d (EofN) and shows the kinematics of Na I D lines (in absorption) and Halpha, 6562.8 A,…

Astrophysics of Galaxies · Physics 2019-08-14 Jose Antonio Garcia-Barreto , Y. Divakara Mayya , Jose Guichard

We present a photometric study of UGC 4599, a low-luminosity galaxy superficially resembling Hoag's Object in that on sky survey images it appears to be a complete ring surrounding a roundish core. The nature of the outer ring of Hoag-type…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Ido Finkelman , Noah Brosch

The spectra of Herbig Haro objects are usually characteristic of ionization and excitation in shock-heated gas, whether an internal shock in an unsteady outflow or a bow shock interface with the interstellar medium. We examine the…

Astrophysics · Physics 2009-11-11 K. P. M. Blagrave , P. G. Martin , J. A. Baldwin

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…

Solar and Stellar Astrophysics · Physics 2016-10-12 L. F. Rodriguez , J. O. Yam , C. Carrasco-Gonzalez , G. Anglada , A. Trejo

We present (sub)millimeter line and continuum observations in a mosaicing mode of the massive star forming region Cepheus A East made with the Submillimeter Array (SMA). Our mosaic covers a total area of about 3$'$ $\times$ 12$'$ centered…

Astrophysics of Galaxies · Physics 2013-05-20 Luis A. Zapata , Manuel Fernandez-Lopez , Salvador Curiel , Nimesh Patel , Luis F. Rodriguez

We present a multi-wavelength study of two HH objects (137 and 138) that may be associated. We use Gemini H$_2$ (2.12 $\mu$m) and K (2.2 $\mu$m) images, as well as APEX molecular line observations and Spitzer image archives. Several H$_2$…

Solar and Stellar Astrophysics · Physics 2020-07-02 Leticia V. Ferrero , Cristina E. Cappa , Hugo P. Saldaño , Mercedes Gómez , Mónica Rubio , Guillermo Güthardt

We investigate the young stellar population in and near the cometary globule Ori,I-2. The analysis is based on deep Nordic Optical Telescope R-band and H-alpha images, JCMT SCUBA 450 and 850 micron images combined with near-infrared 2MASS…

Astrophysics of Galaxies · Physics 2014-11-20 B. Mookerjea , G. Sandell

The bipolar jet HH 212, among the finest collimated jets known, has so far been detected only in near-infrared H$_2$ emission. Here we present deep optical images that show two of the major bow shocks weakly detected in optical [SII]…

Solar and Stellar Astrophysics · Physics 2019-11-20 Bo Reipurth , C. J. Davis , John Bally , A. C. Raga , B. P. Bowler , T. R. Geballe , Colin Aspin , Hsin-Fang Chiang

The core of the nearby galaxy NGC660 has recently undergone a spectacular radio outburst; using a combination of archival radio and Chandra X-ray data, together with new observations, the nature of this event is investigated. Radio…

Astrophysics of Galaxies · Physics 2015-08-06 Megan Argo , Ilse van Bemmel , Sam Connolly , Robert Beswick

We have undertaken high-resolution follow-up of a sample of high velocity HI clouds apparently associated with M31. Our sample was chosen from the population of high-velocity clouds (HVCs) detected out to 50 kpc projected radius of the…

Astrophysics · Physics 2009-11-10 T. Westmeier , R. Braun , D. Thilker

We report high angular resolution observations, made with the Atacama Large Millimeter Array in band 6, of high excitation molecular lines of $\rm CH_3CN$ and $\rm SO_2$ and of the H29$\alpha$ radio recombination line towards the…

The recent detection of X-ray emission from HH 2 and HH 154 with the Chandra and XMM-Newton satellites (respectively) have opened up an interesting, new observational possibility in the field of Herbig-Haro objects. In order to be able to…

Astrophysics · Physics 2009-11-07 A. C. Raga , A. Noriega-Crespo , P. F. Velazquez
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