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arxiv.org arXiv
arxiv.org › abs › 2504.03585v1
We examine the redshift evolution of the relationship between the neutral atomic hydrogen ({\HI}) content and star-formation properties of blue galaxies, along with their location in the cosmic web. U...
arxiv.org arXiv
arxiv.org › abs › 1811.01289v1
Phosphorene is a new two-dimensional material composed of a single or few atomic layers of black phosphorus. Phosphorene has both an intrinsic tunable direct band gap and high carrier mobility values,...
arxiv.org arXiv
arxiv.org › abs › 1406.3477v1
In this chapter we consider two formation channels for blue straggler stars: 1) the merger of two single stars via a collision, and 2) those produced via mass transfer within a binary. We review how c...
arxiv.org arXiv
arxiv.org › abs › 1212.3261v4
It is a classical insight that the Yoneda embedding defines an equivalence of schemes as locally ringed spaces with schemes as sheaves on the big Zariski site. Similarly, the Yoneda embedding identifi...
arxiv.org arXiv
arxiv.org › abs › 2501.11667v1
Eccentric planets may spend a significant portion of their orbits at large distances from their host stars, where low temperatures can cause atmospheric CO2 to condense out onto the surface, similar t...
arxiv.org arXiv
arxiv.org › abs › 1406.3467v1
The old (7 Gyr) open cluster NGC 188 has yielded a wealth of astrophysical insight into its rich blue straggler population. Specifically, the NGC 188 blue stragglers are characterized by: A binary fre...
arxiv.org arXiv
arxiv.org › abs › 1406.3493v1
This chapter explores how we might use the observed {\em statistics} of blue stragglers in globular clusters to shed light on their formation. This means we will touch on topics also discussed elsewhe...
arxiv.org arXiv
arxiv.org › abs › 1406.3463v1
In this chapter, I describe early ideas on blue stragglers, and various observations (some published, some not) that promised but failed to resolve the question of their origin. I review the data and ...
arxiv.org arXiv
arxiv.org › abs › 1406.3491v1
This chapter describes the current state of models of individual blue stragglers. Stellar collisions, binary mergers (or coalescence), and partial or ongoing mass transfer have all been studied in som...
arxiv.org arXiv
arxiv.org › abs › 1406.3475v1
One of the principal mechanisms that is responsible for the origin of blue stragglers is mass transfer that takes place while one of the binary companions overfills its Roche lobe. In this Chapter, we...