Results 161 to 170 of about 49,316 (344)
Explaining the photometric and spectroscopic properties of The Sip-39 galaxy pair
The Sip-39 pair’s galaxies have been investigated using photometric and spectroscopic methods; the observation data was collected from the SDSS's Data Release (DR17) and fitted to ellipses through utilizing the Image Reduction and Analysis Facility ...
Haydar R. Al-baqir, Abdullah K. Ahmed
doaj +1 more source
Shock Excitation in Interacting Galaxies: Markarian 266 [PDF]
R. Davies, M. J. Ward, Hajime Sugai
openalex +1 more source
ABSTRACT When does an agent possess a proposition P as evidence? According to Timothy Williamson, the answer is when, and only when, they know that P. Call this view E = K. In this article, I point out an unwanted consequence of E = K, which is that people who suffer from anxiety have impoverished empirical evidence due to their anxiety.
Rhys Borchert
wiley +1 more source
Caught in the Cosmic Web: Evidence for Ram Pressure Stripping of a Low-mass Galaxy by the Cosmic Web
We present interferometric radio observations of the neutral atomic gas in AGC 727130, a low-mass, gas-rich field galaxy lacking significant star formation.
Nicholas Luber +8 more
doaj +1 more source
An extremely optically dim tidal feature in the gas-rich interacting galaxy group NGC 871/NGC 876/NGC 877 [PDF]
K. Lee-Waddell +9 more
openalex +1 more source
Abstract Introduction Juvenile coral reef fish face an initial predation‐induced mortality bottleneck with mortality exceeding 60% within 48 hours of settlement. This intense predation, exacerbated by anthropogenic stressors, limits recruitment and contributes to global declines of reef fish populations. Post‐Larval Capture, Culture, and Release (PCCR),
Alan Gojanovic +7 more
wiley +1 more source
What Is Heat? Can Heat Capacities Be Negative? [PDF]
Roduner E.
europepmc +1 more source
A dynamical proximity analysis of interacting galaxy pairs [PDF]
Using the impulsive approximation to study the velocity changes of stars during disk-sphere collisions and a method due to Bottlinger to study the post collision orbits of stars, the formation of various types of interacting galaxies is studied as a ...
Chatterjee, Tapan K.
core +1 more source
Young Massive Clusters in Non-Interacting Galaxies [PDF]
Søren S. Larsen +3 more
openalex +1 more source

