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Orion OB1a - the group of stars northwest of the Orion Belt stars with an average age of about 12 million years. Within this grouping is another subgroup known as the 25 Orionis group. [4][5] …

Belonging to the vast Orion OB1 {star_intro.html#assoc">association of hot young stars, 25 Ori was long thought to be part of the Ori OB1a subdivision that consists of the stars up and to the …

25 Orionis is a main sequence star located in the constellation of Orion, The Hunter. It is not part of the Orion constellation outline but is within the borders of the constellation. Based on the …

25 Orionis is the dominant member of a rich low-mass star region, first identified in 2005 in a statistical analysis of 2.5 million stars. It is one of several sub-associations within Orion OB1a, …

Jun 1, 2007 · We report here on the photometric and kinematic properties of a well-defined group of nearly 200 low-mass pre-main-sequence stars, concentrated within ~1° of the early-B star …

hin 1 of the early-B star 25 Ori, in the Orion OB1a subasso. iation. We refer to this stellar aggregate as the 25 Orionis group. The group also harbors the Herbig Ae/Be star V346 Ori …

The 25 Ori stellar aggregate is the most populous ∼ 10 Myr sample yet known within 500 pc, setting it as an excellent laboratory to study the evolution of solar-like stars and protoplanetary …

Jun 20, 2017 · Previous spectroscopic studies have confirmed 160 LMSs in the 25 Orionis stellar group (25 Ori), which is the most prominent overdensity of Orion OB1a. Nonetheless, the …

Jan 24, 2007 · We report here on the photometric and kinematic properties of a well defined group of nearly 200 low-mass pre-main sequence stars, concentrated within ~ 1 deg of the early-B …

We find that the spatial distributions of low-mass stars and brown dwarfs in 25 Orionis are statistically indistinguishable.

Dec 19, 2008 · We report here on the photometric and kinematic properties of a well-defined group of nearly 200 low-mass pre-main-sequence stars, concentrated within ~1° of the early-B …

May 8, 2017 · The Orion OB1a sub-association is a rich low mass star (LMS) region. Previous spectroscopic studies have confirmed 160 LMSs in the 25 Orionis stellar group (25 Ori), which …

The ∼7-10 Myr old stellar group 25 Orionis (25 Ori) is one of the most numerous and spatially dense populations at this age within 400 pc and also presents minimum extinction ( ̄AV ≈ 0.30 …

25 Orionis, less commonly known by its Bayer designation Psi 1 Orionis (ψ 1 Orionis, ψ 1 Ori) is a fifth-magnitude star in the constellation Orion. It lies among a dense cluster of low-mass pre …

We report here on the photometric and kinematic properties of a well defined group of nearly 200 low-mass pre-main sequence stars, concentrated within ~ 1 deg of the early-B star 25 Ori, in …

25 Orionis, less commonly known by its Bayer designation Psi1 Orionis (ψ1 Orionis, ψ1 Ori) is a fifth-magnitude star in the constellation Orion. It lies among a dense cluster of low-mass pre …

Nov 20, 2024 · 25 Orionis, less commonly known by its Bayer designation Psi1 Orionis (1 Orionis, 1 Ori) is a fifthmagnitude star in the constellation Orion. Its kinematics place it among a dense …

We report here on the photometric and kinematic properties of a well-defined group of nearly 200 low-mass pre-main-sequence stars, concentrated within ~1° of the early-B star 25 Ori, in the …

Belatriks je tretja najsvetlejša zvezda in kandidatka za binarno zvezdo ozvezdja Orion, leži 5° zahodno od rdeče superorjakinje Betelgeze (Alfa Orionis). Ima Bayerjevo poimenovanje γ …