Results 171 to 180 of about 453,375 (273)
On powers of the diophantine function $\star:x\mapsto x(x+1)$ [PDF]
We treat the functions $\star^k:{\mathbf N}\rightarrow{\mathbf N}$ where $\star:x\mapsto \star x := x(x+1)$. The set $\{\star^k x+1: \{x,k\}\subseteq{\mathbf N}\}$ is pairwise coprime; so, the set ${\mathbf P}$ of primes is infinite. Our Theorem 4 resorts to the mother sequence, M, that is obtained by factoring the infinite sequence $2,3,4,5,\ldots ...
arxiv
Luminosity jumps in pre-main-sequence stars
Thermal relaxation in young stars is discussed, showing how luminosity jumps occur in those of sufficient mass. The essential character of the thermal relaxation process is shown to be internal heat transfer accompanied by nonhomologous contraction.
openaire +2 more sources
We perform the first magnetic field strength survey of Class I and Flat Spectrum (FS) sources using K -band observations with iSHELL. We obtained new observations of 42 Class I and FS sources and additionally included 10 sources from the archive.
C. Flores+4 more
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EXPORT: Near-IR observations of Vega-type and pre-main sequence stars [PDF]
C. Eiroa+23 more
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Dracula’s Chivito: Discovery of a Large Edge-on Protoplanetary Disk with Pan-STARRS
We report the serendipitous discovery of a large edge-on protoplanetary disk in Pan-STARRS (PS1) images. PS1 has five broadband filters designated as g _P1 , r _P1 , i _P1 , z _P1 , and y _P1 with mean wavelengths 4866, 6215, 7545, 8679, and 9633 Å ...
Ciprian T. Berghea+8 more
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Accretion onto Pre-Main Sequence Binary Stars: The Circumstellar Environment [PDF]
Robert D. Mathieu
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Circumstellar Disks in pre-Main Sequence Stars
This review covers the properties of disks around pre-main--sequence stars. It is at this time in the evolution that planets form, and it is important to understand the properties of these disks to understand planet formation. I discuss disk shapes, masses and temperatures, the properties of the host stars, disk lifetimes and dissipation processes ...
openaire +2 more sources
Spin-down of Solar-mass Protostars in Magnetospheric Accretion Paradigm
Stellar spin is one of the fundamental quantities that characterize a star itself and its planetary system. Nevertheless, stellar spin-down mechanisms in protostellar and pre-main-sequence stellar phases have been a long-standing problem in star ...
Shinsuke Takasao+4 more
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A spectro-astrometric study of southern pre-main sequence stars [PDF]
M. Takami+2 more
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Young associations record complete histories of star-forming events through their demographics and dynamics, and Gaia has greatly expanded our knowledge of these associations.
Ronan Kerr+4 more
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