Results 21 to 30 of about 1,638,100 (309)

Continuum radio emission from the Magellanic Clouds [PDF]

Symposium - International Astronomical Union, 1964
Before discussing the results of the radio observations of the Magellanic Clouds in detail, it is worth while to briefly review some of our current ideas about radio emission from “normal” galaxies which would be the classification given to the Clouds by radio astronomers.
D. S. Mathewson, J. R. Healey
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Radio-continuum emission from the young galactic supernova remnant G1.9+0.3 [PDF]

Serbian Astronomical Journal, 2014
We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of ~181±25 years is the youngest known in the Galaxy.
de Horta A.Y., Filipović M.D., Crawford E.J., Stootman F.H., Pannuti T.G., Bozzetto L.M., Collier J.D., Sommer E.R., Kosakowski A.R.   +8 more
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SYNCHROTRON EMISSION FROM THE GALACTIC HI LAYER [PDF]

Journal of Astronomy and Space Sciences, 2007
The relationship between the Galactic magnetic field strength and the gas density has been revisited. A synchrotron continuum emission data at 408 MHz and HI column density provide a good data for such study.
Yonggi Kim, Jun-Young Oh
doaj   +1 more source

A multi-epoch study of radio continuum emission from massive protostars [PDF]

Monthly Notices of the Royal Astronomical Society, 2020
ABSTRACT We report the results of the Jansky Very Large Array (JVLA) observation of five massive protostars at 6 and 22.2 GHz. The aim of the study was to compare their current fluxes and positions with previous observations to search for evidence of variability.
Obonyo, WO, Lumsden, SL, Hoare, MG, Kurtz, SE, Purser, SJD   +4 more
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Laboratory astrophysics : investigation of planetary and astrophysical maser emission [PDF]

, 2013
This paper describes a model for cyclotron maser emission applicable to planetary auroral radio emission, the stars UV Ceti and CU Virginus, blazar jets and astrophysical shocks.
Ronald K, Phelps, A.D.R., Phelps, Alan, Kellett BJ, McConville SL, Phelps ADR, Speirs DC, Ronald, Kevin, McConville, S.L., Cross, Adrian, Cairns RA, Speirs, D.C., Cairns, R Alan, Cross, A.W., Cross AW, Kellett, Barry, McConville, Sandra, Cairns, R.A., Bingham, Robert, Vorgul I, Vorgul, Irena, Kellett, B.J., Ronald, K., Bingham R, Spiers DC, Vorgul, I., Speirs, David, Bingham, R., K. Ronald, B. J. Kellett, R. Bingham, A. W. Cross, S. L. McConville, I. Vorgul, D. C. Speirs, R. A. Cairns, A. D. R. Phelps   +36 more
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RADIO CONTINUUM EMISSION AND WATER MASERS TOWARD CB 54 [PDF]

The Astronomical Journal, 2009
We present high angular resolution observations of water masers at 1.3 cm and radio continuum emission at 1.3, 3.6 and 6 cm towards the Bok globule CB 54 using the Very Large Array. At 1.3 cm, with subarsecond angular resolution, we detect a radio continuum compact source located to the south-west of the globule and spatially coincident with a mid ...
de Gregorio-Monsalvo, I., Gomez, J. F., Anglada, G., Torrelles, J. M., Kuiper, T. B. H., Suarez, O., Patel, N. A.   +6 more
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Radio Continuum Spectra of Planetary Nebulae

Galaxies, 2018
Radio continuum emission of planetary nebulae is a rich source of information about their structure and physical parameters. Although radio emission is well studied, planetary nebulae show higher spectral indices than expected for homogeneous sphere.
Marcin Hajduk, Peter A. M. van Hoof, Karolina Sniadkowska, Andrzej Krankowski, Leszek Błaszkiewicz, Bartosz Dabrowski, Albert A. Zijlstra   +6 more
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Broadband VLA Spectral-line Survey of a Sample of Ionized Jet Candidates

The Astrophysical Journal Supplement Series, 2023
The study of the interaction between ionized jets, molecular outflows, and their environments is critical to understanding high-mass star formation, especially because jets and outflows are thought to be key in the transfer of angular momentum outward ...
E. Sanchez-Tovar, E. D. Araya, V. Rosero, P. Hofner, S. Kurtz   +4 more
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A global view on star formation: The GLOSTAR Galactic plane survey

Astronomy & Astrophysics
Context. Extended radio continuum emission and its linear polarization play a key role in probing large-scale structures of synchrotron and free-free emission in the Milky Way.
Gong Y., Reich W., Rugel M. R., Menten K. M., Brunthaler A., Wyrowski F., Müller P., Dzib S. A., Urquhart J. S., Yang A. Y., Dokara R., Ortiz-León G. N., Winkel B., Kraus A., Sathyanarayanan S. P., Kim W.-J., Beuther H., Pandian J. D., Cheema A., Khan S., Veena V. S., Roy N., Carrasco-Gonzalez C., Cotton W., Csengeri T., Medina S.-N. X., Nguyen H.   +26 more
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Nonthermal Radio Continuum Emission from Young Nearby Stars

The Astrophysical Journal, 2022
Abstract Young and magnetically active low-mass stars often exhibit nonthermal coronal radio emission owing to the gyration of electrons in their magnetized chromospheres. This emission is easily detectable at centimeter wavelengths with the current sensitivity of large radio interferometers like the Very Large Array (VLA).
Ralf Launhardt, Laurent Loinard, Sergio A. Dzib, Jan Forbrich, Geoffrey C. Bower, Thomas K. Henning, Amy J. Mioduszewski, Sabine Reffert   +7 more
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