University of California’s frontline workers have canceled the
system-wide strike originally planned to begin on Thursday after reaching a tentative agreement with the UC on Wednesday night.
These 42,000 service and patient care workers
— represented by the American Federation of State, County and Municipal Employees Local 3299 (AFSCME)
— have worked without a ratified contract since 2024, due to “stalled” negotiations with the UC, according to union leadership.
…
Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations
Khushboo K. Rao (Institute of Astronomy, National Central University, 300 Zhongda Road, Zhongli 32001 Taoyuan, Taiwan), Sambaran Banerjee (Helmholtz-Instituts f\"ur Strahlen- und Kernphysik)
https://arxiv.org/abs/2607.18681 https://arxiv.org/pdf/2607.18681 https://arxiv.org/html/2607.18681
arXiv:2607.18681v1 Announce Type: new
Abstract: Extended main-sequence turnoffs, extended main sequences, and split main sequences observed in the colour-magnitude diagrams of young and intermediate-age star clusters are now widely interpreted as the consequence of a distribution of stellar rotation rates among their intermediate-mass (1.5-1.8~M$_\odot$) members. However, the origin of the slowly rotating population that occupies the blue main sequence (bMS) remains uncertain, and stellar mergers have been proposed as one possible pathway. We investigate whether stellar mergers can account for the observed bMS population in the 330-Myr Galactic open cluster NGC 3532. We perform fourteen direct NBODY7 simulations spanning different initial cluster masses, radii, binary fractions, and binary orbital distributions. The simulations are selected to reproduce the present-day properties of NGC 3532 within the observational uncertainties, allowing us to estimate the expected number of merger products among its intermediate-mass main-sequence (MS) members. The cluster hosts $\approx 37\%$ bMS members among its intermediate-mass MS population, which are predominantly slow rotators. Despite this large bMS population, our simulations produce only a handful of MS-MS merger products, due to the cluster's low density and substantial mass loss during its evolution. Stellar mergers are unlikely to be the dominant formation channel for the observed slowly rotating bMS population in NGC 3532 and other disperse open clusters. Our results instead favour angular-momentum loss mechanisms operating before or shortly after the zero-age main sequence, such as pre-main-sequence star-disk interactions or tidal synchronization in low-mass ratio binaries.
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🇺🇦 #NowPlaying on BBCRadio3's #ThroughTheNight
Ester Mägi, Academic Male Choir of Tallinn University of Technology, Estonian National Symphony Orchestra & Arvo Volmer:
🎵 Ballad 'Tuule Tuba' (House of Wind)
#EsterMägi
https://open.spotify.com/track/01B4vRPWzWjB0qKxd2Le8I
The 2026 World Congress of Business #History will be held at the University of #Toronto in late July. The organizers have commissioned a #podcast series, produced by recently minted history PhD Louis Reed-Wood, on the university,…
Went to a tour of the University House restoration progress with Peter Kanowski today. Looking really good. Soft open of cellar bar and kitchen in June/July. Public opening on 14/15 August.
#canberra #anu
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Johann Sebastian Bach, Raphael Höhn, Gdansk University Choir & Café Zimmermann:
🎵 Ich armer Mensch, ich Sündenknecht, BWV.55
#JohannSebastianBach #RaphaelHöhn #newRelease 🆕 single
https://open.spotify.com/track/3nHlMwbNMSMW10J392Pd52