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The IRAS source 03256+3055 in the NGC 1333 star forming region is associated with extended sub-millimeter emission of complex morphology, showing multiple clumps. One of these is found to coincide with the driving source of a bipolar jet of…

Astrophysics · Physics 2009-11-10 Klaus W. Hodapp , John Bally , Jochen Eisloeffel , Christopher J. Davis

We model Spitzer Space Telescope observations of the Taurus Class 0 protostar L1527 IRS (IRAS 04368+2557) to provide constraints on its protostellar envelope structure. The nearly edge-on inclination of L1527 IRS, coupled with the highly…

Astrophysics · Physics 2009-11-13 John J. Tobin , Lee Hartmann , Nuria Calvet , Paola D'Alessio

Context. Transition disks (TDs) are circumstellar disks with inner regions highly depleted in dust. TDs are observed in a small fraction of disk-bearing objects at ages of 1-10 Myr. They are important laboratories to study evolutionary…

Earth and Planetary Astrophysics · Physics 2018-07-25 Paola Pinilla , Antonella Natta , Carlo F. Manara , Luca Ricci , Aleks Scholz , Leonardo Testi

Mid-infrared (10-25 \micron) imaging of the protostellar binary system L1448N-IRS3(A,B) is presented. Only one source, IRS3(A), was detected at mid-infrared wavelengths -- all of the mid-infrared emission from IRS3(A,B) emanates from…

Cometary globule 12 is a relatively little investigated medium- and low mass star forming region 210 pc above the Galactic plane. NIR J, H, and Ks imaging and stellar photometry is used to analyse the stellar content and the structure of CG…

Astrophysics of Galaxies · Physics 2015-05-14 Lauri K. Haikala , Bo Reipurth

We have carried out observations of the starless core L1544 in the CCS (J_N=3_2-2_1) line at 9 millimeters wavelength using the BIMA array. The maps show an elongated condensation, 0.15 x 0.045 pc in size, with stronger emission at the…

Astrophysics · Physics 2009-10-31 Nagayoshi Ohashi , Siow Wang Lee , David J. Wilner , Masahiko Hayashi

We investigate the silicate feature of the two Class I components of HH250-IRS, a resolved binary system with a separation of $0''53$ driving a Herbig-Haro flow. Each component has its own circumstellar envelope, and the system is…

Solar and Stellar Astrophysics · Physics 2019-08-21 F. Comerón , B. Merin , B. Reipurth , H. -W. Yen

The interstellar medium (ISM) has a multiphase structure characterized by gas, dust and molecules. The gas can be found in different charge states: neutral, low-ionized (warm) and high-ionized (hot). It is possible to probe the multiphase…

High Energy Astrophysical Phenomena · Physics 2013-02-19 C. Pinto , J. S. Kaastra , E. Costantini , F. Verbunt

We report NIR broad and narrow band photometric observations in the direction of the IRAS17149-3916 source that reveal the presence of a young cluster of massive stars embedded in an HII region coincident with RCW121. These observations,…

Astrophysics · Physics 2008-11-26 Alexandre Roman-Lopes , Zulema Abraham

We present high spatial resolution Submillimeter Array observations and supplementary single-dish photometry of the molecular gas and dust around IRAS 04158+2805, a young source with spectral type M5-M6 in the Taurus star-forming region. A…

Astrophysics · Physics 2009-11-13 Sean M. Andrews , Michael C. Liu , Jonathan P. Williams , K. N. Allers

Stellar fluxes from the 2MASS catalog are used to remove the contribution due to Galactic stars from the intensity measured by DIRBE in four regions in the North and South Galactic polar caps. After subtracting the interplanetary and…

Astrophysics · Physics 2009-10-31 E. L. Wright

We present surface photometry and stellar kinematics of NGC 4264, a barred lenticular galaxy in the region of the Virgo Cluster undergoing a tidal interaction with one of its neighbours, NGC 4261. We measured the bar radius (a_bar=3.2…

High angular resolution H2CO line observations have been carried out for the low mass proto-binary star IRAS 16293-2422 using the OVRO millimeter array. Simultaneous continuum observations reveal that the source most probably contains two…

Astrophysics · Physics 2007-05-23 F. L. Schoeier , J. K. Jorgensen , E. F. van Dishoeck , G. A. Blake

Context. The star HD 87643, exhibiting the "B[e] phenomenon", has one of the most extreme infrared excesses for this object class. It harbours a large amount of both hot and cold dust, and is surrounded by an extended reflection nebula.…

We present an observational study of the protostellar core B335 harboring a low-mass Class 0 source. The observations of the H13CO+(J=1-0) line emission were carried out using the Nobeyama 45 m telescope and Nobeyama Millimeter Array. Our…

Solar and Stellar Astrophysics · Physics 2015-06-15 Yasutaka Kurono , Masao Saito , Takeshi Kamazaki , Koh-Ichiro Morita , Ryohei Kawabe

We present 7 mm, 1.3 cm and 3.6 cm continuum observations made with the Very Large Array toward a sample of ten luminous IRAS sources that are believed to be regions of massive star formation. We detect compact 7 mm emission in four of…

Astrophysics · Physics 2016-08-30 Luis Zapata , Luis Rodriguez , Paul Ho , Henrik Beuther , Qizhou Zhang

L1551 IRS 5 is a FUor-like object located in the Taurus star forming region. We present ALMA 1.3 mm continuum observations using a wide range of baselines. The observations recovered the two circumstellar disks composing the system and, for…

Solar and Stellar Astrophysics · Physics 2019-09-11 Fernando Cruz-Sáenz de Miera , Ágnes Kóspál , Péter Ábrahám , Hauyu Baobab Liu , Michihiro Takami

We have performed mid-IR photometry of the young open cluster NGC 2264 using the images obtained with the Spitzer Space Telescope IRAC and MIPS instruments and present a normalized classification scheme of young stellar objects in various…

Solar and Stellar Astrophysics · Physics 2015-05-13 Hwankyung Sung , John R. Stauffer , Mike S. Bessell

We present subarcsecond resolution dust continuum observations of the protostellar collapse candidate B335 made with the IRAM Plateau de Bure Interferometer at wavelengths of 1.2 and 3.0 mm. These observations probe to < 100 AU size scales…

Astrophysics · Physics 2009-11-10 Daniel W. A. Harvey , David J. Wilner , Philip C. Myers , Mario Tafalla

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…

Solar and Stellar Astrophysics · Physics 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
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