Zobrazeno 1 - 10
of 116
pro vyhledávání: '"85A04"'
Autor:
Huang, Yuxin, Simha, Sunil, Khrykin, Ilya, Lee, Khee-Gan, Prochaska, J. Xavier, Tejos, Nicolas, Bannister, Keith, Barrios, Jason, Chisholm, John, Cooke, Jeff, Deller, Adam, Glowacki, Marcin, Marnoch, Lachlan, Shannon, Ryan, Zhang, Jielai
This paper presents the first public data release (DR1) of the FRB Line-of-sight Ionization Measurement From Lightcone AAOmega Mapping (FLIMFLAM) Survey, a wide field spectroscopic survey targeted on the fields of 10 precisely localized Fast Radio Bu
Externí odkaz:
http://arxiv.org/abs/2408.12864
Autor:
Zhang, Huiming, Cui, Yudong, Huang, Yunlei, Lin, Sujie, Liu, Yihan, Qiu, Zijian, Shao, Chengyu, Shi, Yihan, Xie, Caijin, Yang, Lili
Over the past ten years, several breakthroughs have been made in multi-messenger astronomy. Thanks to the IceCube Neutrino Observatory, the detection of astrophysical neutrinos was proved to be practical. However, no source has been significantly ide
Externí odkaz:
http://arxiv.org/abs/2408.05122
Autor:
Gingold, Harry, Quaintance, Jocelyn
Certain measurements in celestial mechanics necessitate having the origin O of a Cartesian coordinate system (CCS) coincide with a point mass. For the two and three body problems we show mathematical inadequacies in Newton's celestial mechanics equat
Externí odkaz:
http://arxiv.org/abs/2405.15639
Autor:
Gingold, Harry, Quaintance, Jocelyn
This article produces wave equations and constructs traveling wave solutions that are intimately related to Newton's equations of celestial mechanics. The traveling wave solutions are expressed in ``closed form'' in terms of elementary functions. The
Externí odkaz:
http://arxiv.org/abs/2405.13262
When the Galactic Cosmic Rays (GCRs) entering the heliosphere, they encounter the solar wind plasma, and their intensity is reduced, so-called solar modulation. The modulation is caused by the combination of a few factors, such as particle energies,
Externí odkaz:
http://arxiv.org/abs/2303.04460
Autor:
Omerbashich, Mensur
Publikováno v:
Journal of Geophysics 65(1):48-77 (2023) https://n2t.net/ark:/88439/x080008, https://geophysicsjournal.com/article/320
Rather than as a star classically assumed to feature elusive dynamo or a proverbial engine and impulsively alternating polarity, the Sun reveals itself in the 385.8-2.439-nHz (1-mo-13-yr) band of polar ({\phi}Sun>|70{\deg}|) wind's decadal dynamics,
Externí odkaz:
http://arxiv.org/abs/2301.07219
Power spectra of spatial fluctuations of X-ray emission may impose constraints on the origins of the emission independent of that from the energy spectra. We generated spatial power spectrum densities (PSD) of blank X-ray skies observed with Suzaku X
Externí odkaz:
http://arxiv.org/abs/2111.12919
Autor:
Namumba, Brenda, Koribalski, Baerbel Silvia, Józsa, Gyula I. G., Lee-Waddell, Karen, Jones, Michael Gordon, Carignan, Claude, Verdes-Montenegro, Lourdes, Ianjamasimanana, Roger, de Blok, Erwin W. J. G., Cluver, Michelle, Garrido, Julian, Sanchez-Exposito, Susana, Ramaila, Athanaseus, Thorat, Kshitij, Andanti, Lexy A. L., Hugo, Benjamin, Kleiner, Dane, Kamphuis, Peter, Serra, Paolo, Smirnov, Oleg, Maccagni, Filippo, Makhathini, Sphesihle, Molnar, Daniel Csaba Csaba, Perkins, Simon, Ramatsoku, Mpati, White, Sarah V., Loi, Francesca
We report the discovery of large amounts of previously undetected cold neutral atomic hydrogen (\HI) around the core triplet galaxies in the nearby NGC~7232 galaxy group with MeerKAT. With a physical resolution of $\sim$1 kpc, we detect a complex web
Externí odkaz:
http://arxiv.org/abs/2105.10428
Autor:
Couture, Gilles
We study the effects of an encounter between a wandering cosmic object (WCO) of 0.1 solar mass and some Kuiperian Objects (KO). First, we let the WCO cross the out-skirt of ou Kuiper belt. Such encounters can produce two types of solar objects: Eccen
Externí odkaz:
http://arxiv.org/abs/1908.06191
Autor:
Campi, Cristina, Benvenuto, Federico, Massone, Anna Maria, Bloomfield, D Shaun, Georgoulis, Manolis K, Piana, Michele
Solar flares originate from magnetically active regions but not all solar active regions give rise to a flare. Therefore, the challenge of solar flare prediction benefits by an intelligent computational analysis of physics-based properties extracted
Externí odkaz:
http://arxiv.org/abs/1906.12094