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II Zw 40 is a starburst dwarf and merger product, and holds a radio-infrared supernebula excited by thousands of embedded OB stars. We present here observations of three aspects of the supernebula: maps of the K and KU radio continuum that…

Astrophysics of Galaxies · Physics 2024-10-24 Dan Beilis , Sara Beck , John Lacy , Jean L. Turner , Hauyu Baobab Liu , Paul T. P. Ho , S. Michelle Consiglio

We have studied a star-forming complex S193 using near-infrared (NIR) observations and other archival data covering optical to radio wavelengths. We identified stellar clusters in the complex using the NIR photometric data and estimated the…

(Aims): We study the LMC interstellar medium in the field of the nebula N157B, which contains a supernova remnant, an OB association, ionized gas, and high-density dusty filaments in close proximity. We investigate the relative importance…

Astrophysics of Galaxies · Physics 2009-07-17 E. R. Micelotta , B. R. Brandl , F. P. Israel

Aims. We aim to investigate the molecular environment of the supernova remnant (SNR) G150.3+4.5, and explore its association with ambient molecular clouds (MCs). Methods. We present large-field CO (J=1-0) molecular line observations toward…

Astrophysics of Galaxies · Physics 2024-06-26 Jian-Cheng Feng , Xuepeng Chen , Yang Su , Li Sun , Shiyu Zhang , Xin Zhou , Weihua Guo

RCW49 and its ionizing cluster form an extensive, complex region, widely studied at IR and optical wavelengths. Molonglo 843 MHz and ATCA data at 1.4 and 2.4 GHz showed two shells. Recent high-resolution IR imaging revealed a complex dust…

Massive colliding-wind binaries that host a Wolf-Rayet (WR) star present a potentially important source of dust and chemical enrichment in the interstellar medium (ISM). However, the chemical composition and survival of dust formed from…

We report on the detection of HCO+ and 12CO emission in the rotational transition J=1-0 in the vicinity of the shock front at the southern border of the supernova remnant RCW 103, where previous infrared observations suggest an interaction…

Astrophysics · Physics 2009-11-11 S. A. Paron , E. Reynoso , C. Purcell , G. Dubner , A. Green

We present narrow band AAO/UKST HAlpha images and medium and low resolution optical spectra of a nebula shell putatively associated with the Wolf-Rayet star WR 60. We also present the first identification of this shell in the radio regime…

Astrophysics of Galaxies · Physics 2015-05-18 M. Stupar , Q. A. Parker , M. D. Filipovic

We report long-baseline interferometric measurements of circumstellar dust around massive evolved stars with the MIDI instrument on the Very Large Telescope Interferometer and provide spectrally dispersed visibilities in the 8-13 micron…

We present a multiwavelength study of the extended green object, G12.42+0.50 in this paper. The associated ionized, dust, and molecular components of this source are studied in detail employing various observations at near-, mid- and…

Astrophysics of Galaxies · Physics 2019-02-27 Namitha Issac , Anandmayee Tej , Tie Liu , Watson Varricatt , Sarita Vig , Ishwara Chandra C. H. , Mathias Schultheis

Radio and infrared interferometry of SiO maser stars provide complementary information on the atmosphere and circumstellar environment at comparable spatial resolution. Here, we present the latest results on the atmospheric structure and…

Solar and Stellar Astrophysics · Physics 2015-06-04 M. Wittkowski , D. A. Boboltz , M. D. Gray , E. M. L. Humphreys , I. Karovicova , M. Scholz

(abbreviated) We aim to study the inner wind of the well-known AGB star CW Leo. Different diagnostics probing different geometrical scales have pointed toward a non-homogeneous mass-loss process: dust clumps are observed at milli-arcsec…

Solar and Stellar Astrophysics · Physics 2015-01-21 L. Decin , A. M. S. Richards , D. Neufeld , W. Steffen , G. Melnick , R. Lombaert

We examine the new Galactic supernova remnant (SNR) candidate, G23.11+0.18, as seen by the Murchison Widefield Array (MWA) radio telescope. We describe the morphology of the candidate and find a spectral index of -0.63+/-0.05 in the…

We present a detailed analysis of high resolution near-infrared imaging and spectroscopy of the potential star cluster IRS13E very close to the massive black hole in the Galactic Center. We detect 19 objects in IRS13E from Ks-band images,…

We have spectroscopically discovered a pair of twin, nitrogen-type, hydrogen-rich, Wolf-Rayet stars (WN8-9h) that are both surrounded by circular, mid-infrared-bright nebulae detected with the Spitzer Space Telescope and MIPS instrument.…

Solar and Stellar Astrophysics · Physics 2015-05-19 Jon Mauerhan , Stefanie Wachter , Pat Morris , Schuyler Van Dyk , D. W. Hoard

We report the results obtained from a multi-wavelength study of the HII region, G18.148$-$0.283, using the upgraded Giant Metre-wave Radio Telescope (uGMRT) at 1350 MHz along with other archival data. In addition to the radio continuum…

Astrophysics of Galaxies · Physics 2022-01-28 Jyotirmoy Dey , Jagadheep D. Pandian , Dharam Vir Lal

We report the discovery of a pair of infrared, axisymmetric rings in the planetary nebula NGC 1514 during the course of the WISE all-sky mid-infrared survey. Similar structures are seen at visible wavelengths in objects such as the…

Astrophysics of Galaxies · Physics 2010-11-18 Michael E. Ressler , Martin Cohen , Stefanie Wachter , D. W. Hoard , Amy K. Mainzer , Edward L. Wright

We report the discovery of a synchrotron nebula, G283.1-0.59, associated with PSR J1015-5719. Radio observations using the Molonglo Observatory Synthesis Telescope and the Australia Telescope Compact Array at 36, 16, 6, and 3 cm reveal a…

High Energy Astrophysical Phenomena · Physics 2017-06-28 C. -Y. Ng , R. Bandiera , R. W. Hunstead , S. Johnston

Stellar population and the interstellar gas-dust medium in the vicinity of the open star cluster vdB 130 are analysed using optical observations taken with the 6-m telescope of the SAO RAS and the 125-cm telescope of the SAI MSU along with…

The volume around the SN 1987A contains a variety of structures, including but certainly not limited to the three-ring nebula glowing in recombination lines. Many of these structures are revealed by light echoes, hence have been mapped in…

Astrophysics · Physics 2007-05-23 Arlin Crotts
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