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www.reddit.com Reddit
reddit.com › r › Brian...s_with_links_to_all ›
Seeing that there is still a lot of misinformation circulating and the NYPD's official timeline has left out certain details, I’ve put together a full timeline of all confirmed events that happened ...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 9912047v2
High-resolution, CO(1-0) interferometry of the ultraluminous infrared galaxy IRAS 14348-1447 is presented. The merger system has a molecular gas mass of \~3x10^10 solar masses and a projected nuclear ...
www.reddit.com Reddit
reddit.com › r › Youth...he_genocide_in_gaza ›
What is happening in Palestine is obivously, genocide. Many of you may not want to see or admit it but we are currently witnessing the the most recorded genocide in human history
Let's start with how...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0110452v1
We present the main results from our 940 ksec observation of the Chandra Deep Field South (CDFS), using the source catalog described in an accompanying paper (Giacconi et al. 2001). We extend the meas...
arxiv.org arXiv
arxiv.org › abs › 1003.5204v1
After leaving the main sequence, massive stars undergo complex evolution, still poorly understood. With a population of 100s OB stars, the starburst cluster Westerlund~1 offers an unparallelled enviro...
arxiv.org arXiv
arxiv.org › abs › hep-ph › 9903290v1
We utilize non-perturbative and fully relativistic methods to calculate the\thinspace \thinspace $ΔNγ$ electromagnetic transition amplitudes $G_{M}^{*}(q^{2})$ (related to the magnetic dipole moment...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0509796v1
We report results from a spectral and timing analysis of M82 X-1, one of the brightest known ultraluminous X-ray sources. Data from a new 105 ks {\it XMM-Newton} observation of M82 X-1, performed in A...
arxiv.org arXiv
arxiv.org › abs › math-ph › 0101033v1
A system of differential forms will establish a topology and a topological structure on a domain of independent variables such that is possible to determine which maps or processes acting on the syste...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0408290v2
We present the analysis of the X-ray Multi-Mirror Mission (XMM-Newton) European Photon Imaging Camera (EPIC) data of the Galactic supernova remnant (SNR) CTB 109 (G109.1-1.0). CTB 109 is associated wi...
arxiv.org arXiv
arxiv.org › abs › 0811.4053v1
Nuclear electron capture rate from continuum in an astrophysical plasma environment (like solar core) is calculated using a modified Debye-Huckel screening potential and the related non-Gaussian q-dis...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0306446v1
We identified star clusters in archived HST/WFPC2 images of the merger and ultra-luminous infrared galaxy NGC 6240, with the aim of investigating whether star cluster properties (luminosity, age and m...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0503615v1
Using the theoretical stellar population synthesis models of BC96, Kong et al. (2003) showed that some BATC colors and color indices could be used to disentangle the age and metallicity effect. They f...