The range of accretion rates between the stellar disks also widens over time, such that after 5000 yr the total disk mass of the fastest-accreting halo from Stacy & Bromm ( 2013

• Abstract machine with many features of computer • Designed before the stored program computer. • No

Here we present a model for the formation of GCs, where low-mass pre-main-sequence stars accrete enriched material released from interacting massive binary and rapidly rotating stars

Students on warning status are still eligible to receive financial aid, but are required to earn a cumulative GPA of at least 2.0 and meet pace requirements (67% completion rate

Finally, a large sample of ultracool binary orbits will provide constraints on formation models for low-mass stars and brown dwarfs as the orbital parameters of binaries

The more luminous Cepheids (W vir star s) are identified with stars undergoing blueward loops from the second giant branch in response to helium shell flashes

INDEX WORDS: Astronomy, Astrometry, Photometry, Spectroscopy, Kinematics, Proper motion, Parallax, Nearby stars, Low-mass stars, Young stars, Pre-main-sequence

It is evident that any specific Aboriginal and Torres Strait Islander maternity program should include care from Aboriginal and Torres Strait Islander health professionals

To see if planet formation processes can alleviate the dust budget crisis without grain growth, we consider dust produced by low-intermediate mass stars and SNe in the

PRESENT: Participants included Kelle Little, Coquille Indian Tribe Community Health Center; Fauna Larkin, Coquille Indian Tribe Community Health Center; Bailey Burkhalter,

In combination, the D rift - M arcs code that we here have presented for the first time, is able to compute self-consistent model atmospheres that can include both

Low-mass Eclipsing Binaries in the Catalina Sky Survey Low-mass EB systems are interesting for determining the fundamental parameters of low-mass stars, which are the most common

large cluster of lower-mass stars around them is a key test in the di ff erentiation of star formation theories as well as how the initial mass function of stars is sampled.

To characterize the evolution of magnetic activity in low-mass stars over their first ≈600 Myr, we consolidate X-ray and optical data from the literature for stars in six other

Distributions of lookback times corresponding to the formation of the youngest 30 per cent of stars for high (dashed lines) and low (solid lines) stellar mass galaxies with discs

Emphasis is placed on the following topics: the solar abundance problem, mass loss on the red giant branch, and the level of helium enrichment associated to the multiple

Key words infrared: stars, stars: binaries: spectroscopic, stars: low-mass, brown dwarfs, techniques: spectroscopic The transition between the L dwarf and T dwarf spectral classes