Results 81 to 90 of about 440 (199)

A New Type of Jovian Hectometric Radiation Powered by Monoenergetic Electron Beams

open access: yesJournal of Geophysical Research: Space Physics, Volume 129, Issue 5, May 2024.
Abstract In this study, we statistically analyze the Jovian auroral radio sources detected in situ by Juno/Waves at frequencies f below the electron cyclotron frequency fce. We first conduct a survey of Juno/Waves data over 1–40 MHz from 2016 to 2022. The 15 detected HectOMetric (HOM) sources all lie within 1–5 MHz and are both less frequent than the ...
B. Collet   +7 more
wiley   +1 more source

FIRST INTERFEROMETRIC IMAGES OF THE 36 GHz METHANOL MASERS IN THE DR21 COMPLEX

open access: yes, 2010
Class I methanol masers are believed to be produced in the shock-excited environment around star-forming regions. Many authors have argued that the appearance of various subsets of class I masers may be indicative of specific evolutionary stages of star ...
Pihlström, Ylva M.   +12 more
core   +1 more source

The distance to G59.7+0.1 [PDF]

open access: yes, 2007
We have measured the distance to the high-mass star-forming region G59.7+0.1, which harbors the far-infra-red source IRAS 19410+2336. The distance is 2.20 ± 0.11 kpc and was determined by triangulation using Very Long Baseline Array (VLBA) observations ...
Reid, M. J.   +5 more
core   +1 more source

Testing OH Megamaser Identification Methods in H i Surveys: Updated Source-flagging Algorithms and New Detections in ALFALFA

open access: yesThe Astrophysical Journal
OH megamasers (OHMs) are extragalactic masers found primarily in gas-rich galaxy major mergers. To date, only ∼120 OHMs have been cataloged since their discovery in 1982, and efforts to identify distinct characteristics of OHM host galaxies have remained
Hayley Roberts   +5 more
doaj   +1 more source

Feasibility of Passive Sounding of Uranian Moons Using Uranian Kilometric Radiation

open access: yesEarth and Space Science, Volume 11, Issue 2, February 2024.
Abstract We present a feasibility study for passive sounding of Uranian icy moons using Uranian Kilometric Radio (UKR) emissions in the 100–900 kHz band. We provide a summary description of the observation geometry, the UKR characteristics, and estimate the sensitivity for an instrument analogous to the Cassini Radio Plasma Wave Science (RPWS) but with
A. Romero‐Wolf   +8 more
wiley   +1 more source

EXPANDED VERY LARGE ARRAY DETECTION OF 44.1 GHz CLASS I METHANOL MASERS IN SAGITTARIUS A

open access: yes, 2011
We report on the detection of 44 GHz Class I methanol (CH[subscript 3]OH) maser emission in the Sagittarius A (Sgr A) complex with the Expanded Very Large Array (EVLA).
Sjouwerman, L. O.   +5 more
core   +1 more source

Surveys of the Milky Way and Magellanic System in the λ21-cm line of atomic hydrogen

open access: yesEPJ Web of Conferences, 2012
In the next three years, surveys of the Northern and Southern skies using focal plane arrays on aperture synthesis radio telescopes will lead to a breakthrough in our knowledge of the warm and cool atomic phases of the interstellar medium and their ...
Dickey J.M.
doaj   +1 more source

Proper Motion of Water Masers Associated with IRAS 21391+5802: Bipolar Outflow and an AU‐Scale Dusty Circumstellar Shell

open access: yes, 2017
We present VLBA observations of water maser emission associated with the star forming region IRAS 21391+5802, which is embedded in a bright rimmed cometary globule in IC1396.
Zhang, Qizhou   +6 more
core   +1 more source

Dynamics of SiO Masers around VX Sgr

open access: yes, 2018
We performed Very Long Baseline Array (VLBA) observations of SiO masers ( ) toward VX Sgr from 2006 July to 2008 August. With the application of a phase reference technique, the accurate relative positions of maser spots at the two transitions can ...
Jiang,D. R.   +3 more
core   +1 more source

The parallax and 3D kinematics of water masers in the massive star-forming region G034.43+0.24

open access: yes, 2023
We report a trigonometric parallax measurement of 22 GHz water masers in the massive star-forming region G034.43+0.24 as part of the Bar and Spiral Structure Legacy (BeSSeL) Survey using the Very Long Baseline Array. The parallax is 0.330$\pm$50.018 mas,
Reid, M. J.   +29 more
core   +1 more source

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