Massive
...
dmfay/massive-js
A data mapper for Node.js and PostgreSQL. (⭐ 2477)
massive adjective - Definition, pictures, pronunciation and usage notes ...
Definition of massive adjective in Oxford Advanced Learner's Dictionary. Meaning, pronunciation, picture, example sentences, grammar, usage notes, synonyms and more.
MASSIVE | English meaning - Cambridge Dictionary
MASSIVE definition: 1. very large in size, amount, or number: 2. a group of people who spend time together and live in…. Learn more.
FransBouma/Massive
A small, happy, dynamic MicroORM for .NET that will love you forever. (⭐ 1799)
The nightmare scenario: measuring the stochastic gravitational-wave background from stalli…
Massive black-hole binaries, formed when galaxies merge, are among the primary sources of gravitational waves targeted by ongoing Pulsar Timing Array (PTA) experiments and the upcoming space-based LISA interferometer. However, their formation and mer...
Say Cheese: a snapshot of the massive DDoS attacks coming from IoT cameras
Points: 336 | Comments: 208 | Author: jgrahamc
nilpunch/massive-ecs
Bitset-based ECS with rollbacks. C# library and Unity package. (⭐ 194)
X-Shooting ULLYSES: Massive stars at low metallicity VI. Atmosphere and mass-loss properti…
Mass loss through a stellar wind is an important physical process that steers the evolution of massive stars and controls the properties of their end-of-life products, such as the supernova type and the mass of compact remnants. For an accurate mass...
A Remarkably Loud Quasi-Periodicity after a Star is Disrupted by a Massive Black Hole
The immense tidal forces of massive black holes can rip apart stars that come too close to them. As the resulting stellar debris spirals inwards, it heats up and emits x-rays when near the black hole. Here, we report the discovery of an exceptionally...
Searching for Magnetic Fields in the Descendants of Massive OB Stars
We present the results of a recent survey of cool, late-type supergiants - the descendants of massive O- and B-type stars - that has systematically detected magnetic fields in these stars using spectropolarimetric observations obtained with ESPaDOnS...
Volume Density Thresholds for Overall Star Formation imply Mass-Size Thresholds for Massiv…
We aim at understanding the massive star formation (MSF) limit $m(r) = 870 M_{\odot} (r/pc)^{1.33}$ in the mass-size space of molecular structures recently proposed by Kauffmann & Pillai (2010). As a first step, we build on the hypothesis of a volume...
The Formation of Massive Stars by Accretion Through Trapped Hypercompact HII Regions
The formation of massive stars may take place at relatively low accretion rates over a long period of time if the accretion can continue past the onset of core hydrogen ignition. The accretion may continue despite the formation of an ionized HII re...
The Decrease of Specific Angular Momentum and the Hot Toroid Formation: The Massive Clump…
This is the first paper of our series of high resolution (1") studies of the massive star forming region G10.6--0.4. We present the emission line observations of the hot core type tracers (O$^{13}$CS, OCS, SO$_{2}$) with $\sim$0$"$.5 resolution. By c...
Speed of sound in dense matter and two families of compact stars
The existence of massive compact stars $(M\gtrsim 2.1 M_{\odot})$ implies that the conformal limit of the speed of sound $c_s^2=1/3$ is violated if those stars have a crust of ordinary nuclear matter. Here we show that, if the most massive objects ar...
A relativistic jetted outburst from a massive black hole fed by a tidally disrupted star
While gas accretion onto some massive black holes (MBHs) at the centers of galaxies actively powers luminous emission, the vast majority of MBHs are considered dormant. Occasionally, a star passing too near a MBH is torn apart by gravitational forces...
Rachael Ray Unrecognizable After Massive Weight Loss, Pic
Feb 22, 2026 · Former Food Network star Rachael Ray hosted an event over the weekend that left fans shocked at her massive weight loss.
On the stunning abundance of super-early, massive galaxies revealed by JWST
The earliest JWST observations have revealed an unexpected abundance of super-early ($z>10$), massive ($M_*\approx 10^9\, M_\odot$) galaxies at the bright-end ($M_{\rm UV}\approx -21$) of the ultraviolet luminosity function (UV LF). We present a mini...
TYC 3340-2437-1: A Quadruple System with A Massive Star
Hierarchical massive quadruple systems are ideal laboratories for examining the theories of star formation, dynamical evolution, and stellar evolution. The successive mergers of hierarchical quadruple systems might explain the mass gap between neutro...
Aspects of Favorable Propagation in Massive MIMO
Favorable propagation, defined as mutual orthogonality among the vector-valued channels to the terminals, is one of the key properties of the radio channel that is exploited in Massive MIMO. However, there has been little work that studies this topic...