Results 11 to 20 of about 1,150 (163)

Accretion-induced variability links young stellar objects, white dwarfs, and black holes. [PDF]

open access: yesSci Adv, 2015
Scaringi S   +8 more
europepmc   +2 more sources

Cyanopolyyne Chemistry around Massive Young Stellar Objects [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract Recent radio astronomical observations have revealed that HC5N, the second shortest cyanopolyyne (HC2n+1N), is abundant around some massive young stellar objects (MYSOs), which is not predicted by classical carbon-chain chemistry.
Kotomi Taniguchi   +5 more
openaire   +3 more sources

Infrared Interferometric Observations of Young Stellar Objects [PDF]

open access: yesThe Astrophysical Journal, 2000
We present infrared observations of four young stellar objects using the Palomar Testbed Interferometer (PTI). For three of the sources, T Tau, MWC 147 and SU Aur, the 2.2 micron emission is resolved at PTI's nominal fringe spacing of 4 milliarcsec (mas), while the emission region of AB Aur is over-resolved on this scale.
Akeson, R. L.   +4 more
openaire   +2 more sources

The GRAVITY young stellar object survey

open access: yesAstronomy & Astrophysics, 2019
Contexto. Los estudios de la distribución del polvo, la composición y la evolución de los discos protoplanetarios proporcionan pistas para comprender la formación de planetas. Sin embargo, se sabe poco sobre las regiones más internas de los discos donde se espera que se formen los planetas telúricos. Objetivos.
Y.-I. Bouarour   +56 more
openaire   +1 more source

Photometric variability of massive young stellar objects [PDF]

open access: yesAstronomy & Astrophysics, 2018
The Vista Variables in the Via Lactea (VVV) survey has allowed for an unprecedented number of multi-epoch observations of the southern Galactic plane. In a recent paper, 13 massive young stellar objects (MYSOs) have already been identified within the highly variable (ΔKs > 1 mag) YSO sample of another published work.
Teixeira, G. D. C.   +10 more
openaire   +3 more sources

The Nature of Blue Stars with Mid-infrared Excesses in the Large Magellanic Cloud

open access: yesThe Astrophysical Journal Supplement Series, 2023
We present low-resolution optical spectra and classifications of 92 blue objects with mid-infrared excesses in the Large Magellanic Cloud. The majority of these objects were selected with the criteria of U − B < 0 and V < 17 from the potential young ...
Ryoko Ishioka   +5 more
doaj   +1 more source

Salt-bearing Disk Candidates around High-mass Young Stellar Objects

open access: yesThe Astrophysical Journal, 2023
Molecular lines tracing the orbital motion of gas in a well-defined disk are valuable tools for inferring both the properties of the disk and the star it surrounds. Lines that arise only from a disk, and not also from the surrounding molecular cloud core
Adam Ginsburg   +8 more
doaj   +1 more source

300: An ACA 870 μm Continuum Survey of Orion Protostars and Their Evolution

open access: yesThe Astrophysical Journal, 2023
We present an 870 μ m continuum survey of 300 protostars from the Herschel Orion Protostar Survey using the Atacama Compact Array (ACA). These data measure protostellar flux densities on envelope scales ≤8000 au (20″) and resolve the structure of ...
Samuel Federman   +13 more
doaj   +1 more source

An APEX Study of Molecular Outflows in FUor-type Stars

open access: yesThe Astrophysical Journal, 2023
The FU Orionis–type objects (FUors) are low-mass pre-main-sequence objects that go through a short-lived phase (∼100 yr) of increased mass accretion rate (from 10 ^−8 to 10 ^−4 M _⊙ yr ^−1 ).
Fernando Cruz-Sáenz de Miera   +6 more
doaj   +1 more source

The GRAVITY young stellar object survey

open access: yesAstronomy & Astrophysics, 2021
Context. 51 Oph is a Herbig Ae/Be star that exhibits strong near-infrared CO ro-vibrational emission at 2.3 μ m, most likely originating in the innermost regions of a circumstellar disc. Aims. We aim to obtain the physical and geometrical properties of the system by spatially resolving the circumstellar environment of the inner gaseous disc.
Koutoulaki, M.   +70 more
openaire   +3 more sources

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