Results 11 to 20 of about 1,638,100 (309)

H i 21 cm Extended Structures to the Northeast and Southwest of NGC 5595: VLA Observations of the Disk Galaxy Pair NGC 5595 and NGC 5597

open access: yesThe Astronomical Journal, 2023
We report VLA B-configuration observations of the H i 21 cm line on the close disk galaxy pair NGC 5595 and NGC 5597. At the angular resolution of the observations, ∼7.″1 × 4.″2, while most of the H i 21 cm in NGC 5595 and NGC 5597 has the same extent as
J. Antonio Garcia-Barreto   +1 more
doaj   +1 more source

First Detection of Radio Emission Associated with a Classical Cepheid

open access: yesThe Astronomical Journal, 2023
We report the detection of 15 GHz radio continuum emission associated with the classical Cepheid variable star δ Cephei ( δ Cep) based on observations with the Karl G. Jansky Very Large Array.
L. D. Matthews, N. R. Evans, M. P. Rupen
doaj   +1 more source

Multifrequency radio observations of SNR J0536-6735 (N 59B) with associated pulsar [PDF]

open access: yesSerbian Astronomical Journal, 2012
We present a study of new Australian Telescope Compact Array (ATCA) observations of supernova remnant, SNR J0536-6735. This remnant appears to follow a shell morphology with a diameter of D=36x29 pc (with 1 pc uncertainty in each direction ...
Bozzetto L.M.   +4 more
doaj   +1 more source

Radio continuum emission of the Milky Way and nearby galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1985
The radio continuum emission of the Milky Way and nearby galaxies can be decomposed into a central region, a clumpy “thin disk”, concentrated in the spiral arms, and a smooth “thick disk” (or flattened “halo”). The emissivity ratio of the two disks seems to be related to the magnetic field properties: Galaxies with strong radio spiral arms reveal a ...
Rainer Beck, Wolfgang Reich
openaire   +1 more source

Radio Continuum Emission in Polar Ring Galaxies

open access: yesThe Astronomical Journal, 2004
We have used the Very Large Array aperture synthesis telescope to conduct a radio continuum survey of polar-ring galaxies, at 20cm and 6cm. Forty objects were observed at 20cm with 5" resolution. Twenty (50%) of the program sources were detected at 20cm, down to our 5-sigma limit of 0.5 mJy/beam.
Cox, A. L., Sparke, L. S.
openaire   +2 more sources

Probing the Interplay between Jets, Winds, and Multi-phase Gas in 11 Radio-quiet PG Quasars: A uGMRT-VLA Study

open access: yesThe Astrophysical Journal, 2023
We present polarization-sensitive images from the Karl G. Jansky Very Large Array (VLA) at 5 GHz of 11 radio-quiet PG quasars. Based on the radio morphology, spectral index, and polarization properties from the VLA study, coupled with the findings of our
Silpa S.   +3 more
doaj   +1 more source

Study of nonthermal continuum patches : wave propagation and plasmapause study [PDF]

open access: yes, 2011
Nonthermal continuum (NTC) radiation is believed to be emitted at the plasmapause and near the magnetic equator. We present a particular type of NTC radiation, referred to as NTC patch, which appears over a wide frequency range and within a relatively ...
P. M. E. Décréau   +18 more
core   +1 more source

Observations of Radio Continuum Emission from M 31 [PDF]

open access: yesSymposium - International Astronomical Union, 1970
Observations of continuum emission from M 31 have been made with the Cambridge One-mile radio telescope (Pooley, 1969). Two observing frequencies were used; maps of the whole of the visible nebula were obtained at 408 MHz, and spectral data for the central region at 1407 MHz.
openaire   +1 more source

Baldwin Effect and Additional BLR Component in AGN with Superluminal Jets

open access: yesFrontiers in Astronomy and Space Sciences, 2016
We study the Baldwin Effect (BE) in 96 core-jet blazars with optical and ultraviolet spectroscopic data from a radio-loud AGN sample obtained from the MOJAVE 2cm survey.
Víctor Manuel Patiño Álvarez   +7 more
doaj   +1 more source

Evidence for Low-power Radio Jet–ISM Interaction at 10 pc in the Dwarf AGN Host NGC 4395

open access: yesThe Astrophysical Journal, 2023
Black-hole-driven outflows in galaxies hosting active galactic nuclei (AGN) may interact with their interstellar medium (ISM) affecting star formation (SF).
Payel Nandi   +12 more
doaj   +1 more source

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