Results 21 to 30 of about 2,374 (304)

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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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
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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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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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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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Radio-continuum emission from quasar host galaxies

The Astronomical Journal, 1987
Seven low-redshift quasars that are likely to be in spiral galaxies have been observed in a search for radio-continuum emission from the host galaxies of quasars. The properties of the individual quasars are listed, and 1.49 GHz contour maps of the seven quasar fields are presented.
J. J. Condon, Ann C. Gower, J. B. Hutchings   +2 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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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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Detection of continuum radio emission associated with Geminga [PDF]

Monthly Notices of the Royal Astronomical Society: Letters, 2011
Abstract A deep Very Large Array observation of the Geminga pulsar field led to the discovery, at a higher than 10σ significance level, of radio emission trailing the neutron star proper motion. This ∼10 arcsec long radio feature, detected with a flux of ∼0.4 mJy at 4.8 GHz, is marginally displaced (2.7 ± 1.8 arcsec) from the pulsar ...
Pellizzoni, A., Govoni, F., Esposito, P., Murgia, M., Possenti, A.   +4 more
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Radio Emission of Nearby Early-type Galaxies in the Low and Very Low Radio Luminosity Range

The Astrophysical Journal, 2023
We analyze radio continuum emission of early-type galaxies with dynamical measurements of central supermassive black hole (SMBH) masses and well-characterized large-scale environments, but regardless of the exact level of the nuclear activity.
Anna Wójtowicz, Łukasz Stawarz, C. C. Cheung, Norbert Werner, Dominik Rudka   +4 more
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