Results 41 to 50 of about 10,468 (212)

Parallax and Distance Estimates for Fourteen Cataclysmic Variable Stars

open access: yes, 2003
I used the 2.4 m Hiltner telescope at MDM Observatory in an attempt to measure trigonometric parallaxes for 14 cataclysmic variable stars. Techniques are described in detail.
Bailey J.   +17 more
core   +1 more source

Advancing Robust Governance in Turbulent Times: The Role of Multi‐Level Governance, Hybrid Governance, and Negotiated Societal Intelligence

open access: yesPublic Administration, EarlyView.
ABSTRACT New research argues that robust governance based on flexible adaptation and proactive innovation is needed in order to uphold core public functions, purposes, and values in times of societal turbulence. However, we have limited knowledge of the conditions for enhancing robust governance.
Jacob Torfing   +9 more
wiley   +1 more source

[PK2008] HalphaJ115927 and IGR J14091-6108: Two New Intermediate Polars Above the Period Gap

open access: yesThe Astronomical Journal
This study presents a detailed timing analyses of two cataclysmic variables (CVs), [PK2008] HalphaJ115927 and IGR J14091-6108, utilizing the optical data from the Transiting Exoplanet Survey Satellite.
Arti Joshi
doaj   +1 more source

On the orbital period of the cataclysmic variable RZ Leonis [PDF]

open access: yes, 2001
In this research note we present a time-resolved study of the Balmer emission lines of RZ Leo. From the analysis of the radial velocities we find an orbital period of 0.07651(26) d.
C. Tappert .,   +6 more
core   +2 more sources

Teaching New Religious Movements Historically: Distance, Empathy, and Cults in the Classroom

open access: yesTeaching Theology &Religion, EarlyView.
ABSTRACT Resistance to understanding the beliefs of modern New Religious Movements (NRMs) is well‐known to those who teach in the area. This paper builds on Eugene Gallagher's repurposing of “methodological belief” for college classes on NRMs by suggesting that scholars and teachers in the field of religious studies engage methods and content drawn ...
Douglas FitzHenry Jones
wiley   +1 more source

OBSERVATIONS OF CATACLYSMIC VARIABLES AT KOLONICA OBSERVATORY

open access: yesOdessa Astronomical Publications, 2007
We present a small sample of our observations of cataclysmic variable stars obtained at Kolonica Observatory, The presented data for CI UMa, MR UMa and SW UM were obtained in 2006 and 2007. Our observations demonstrate that also the small telescopes with
S. Parimucha, P. Dubovsky, I. Kudzej
doaj   +1 more source

Hibernation Revived by Weak Magnetic Braking [PDF]

open access: yes, 2006
Cataclysmic variables undergo periodic nova explosions during which a finite mass of material is expelled on a short timescale. The system widens and, as a result, the mass-transfer rate drops.
Martin, Rebecca G., Tout, Christopher A.
core   +3 more sources

The Perils of Climate Catastrophism: A Call to Situate Crisis and Change

open access: yesWIREs Climate Change, Volume 17, Issue 3, May/June 2026.
Original image taken by John Englart and published on Flickr (https://flickr.com/photos/81043308@N00/33366528414) and then subsequently on Wikipedia (https://commons.wikimedia.org/wiki/File:Climate_emergency_‐_Melbourne_‐MarchforScience_on_‐Earthday_(33366528414).jpg) under the Creative Commons Attribution‐Share Alike 2.0 Generic license.
Karen Bickerstaff
wiley   +1 more source

TESS Light Curves of Cataclysmic Variables. VI. Intermediate Polars

open access: yesThe Astrophysical Journal Supplement Series
The long and (almost) continuous high-cadence light curves provided by the TESS space mission are ideally suited to study in detail brightness variations in stellar sources on the broad range of timescales between minutes and months.
Albert Bruch
doaj   +1 more source

LAMOST J2043+3413—a Fast Disk Precession SW Sextans Candidate in Period Gap

open access: yesThe Astronomical Journal, 2023
We present follow-up photometric observations and time-series analysis of a nova-like, SW Sextans-type, cataclysmic variable (CV) candidate, LAMOST J204305.95+341340.6 (hereafter J2043+3413), with a Gaia G -band magnitude of 15.30 and a distance of 990 ...
Xin Li   +7 more
doaj   +1 more source

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