Results 131 to 140 of about 50,898 (280)
Journal of Management Studies, EarlyView.Abstract Scholars have long attended to both the persistence and change of institutional logic–identity constellations, but we know less about why and how organizational members might cling to a logic despite its evident maladaptive character and the resulting emotional upheaval.
Lindie Botha, Ralph Hamann
wiley +1 more source
Chondrule Survivability in the Solar Nebula
The Astrophysical JournalThe lifetime of millimeter-sized dust grains, such as chondrules, in the nominal solar nebula model is limited to ∼10 ^5 yr, due to an inward drift driven by gas drag.
Tetsuo Taki, Shigeru Wakita
doaj +1 more source
A Surface Reading of Vladimir Nabokov
Critical Quarterly, EarlyView.
Aleksandra Violana
wiley +1 more source
On the character of the chief line of the Nebula in Orion [PDF]
, 1891 K. D. Naegamvala
openalex +1 more source
LBV (Candidate) Nebulae: Bipolarity and Outflows [PDF]
arXiv, 2002 The most massive evolved stars (above 50 M_sun) undergo a phase of extreme mass loss in which their evolution is reversed from a redward to a blueward motion in the HRD. In this phase the stars are known as Luminous Blue Variables (LBVs) and they are located in the HRD close to the Humphreys-Davidson limit.
arxiv
On the Spectrum of the Great Nebula in Orion, and on the Motions of some Stars Towards or from the Earth* [PDF]
, 1872 openalex +1 more source
Multi‐isotope (N, O, Ti, and Cr) study of C1 and CM‐like clasts—Probing unsampled C1 material
Meteoritics &Planetary Science, EarlyView.Abstract A multi‐element isotope (N, O, Ti, and Cr) study was conducted on C1 and CM‐like clasts hosted in achondrites and chondrite breccias to understand the genesis of these chondritic clasts. The mineralogy, O, and N isotopes confirm that CM‐like clasts in howardites and polymict eucrites closely resemble CM chondrite‐like material.
Markus Patzek +9 more
wiley +1 more source
Ring Nebulae around Massive Stars throughout the HR Diagram [PDF]
arXiv, 2002 Massive stars evolve across the HR diagram, losing mass along the way and forming a variety of ring nebulae. During the main sequence stage, the fast stellar wind sweeps up the ambient interstellar medium to form an interstellar bubble. After a massive star evolves into a red giant or a luminous blue variable, it loses mass copiously to form a ...
arxiv