Results 41 to 50 of about 241,576 (378)

Walkaway Star Candidates in IC 348 and Their Possible Birthplaces

open access: yesThe Astrophysical Journal, 2023
Observations and theories reveal that star-forming regions eject their members during the early evolution of the cluster. We present an initial search for stars ejected from the young cluster IC 348 based on an analysis of Gaia EDR3 astrometry of ...
Xingyu Zhou   +4 more
doaj   +1 more source

Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. V. Recent Star Formation in the 30 Dor Nebula [PDF]

open access: yes, 2017
We report on the properties of the low-mass stars that recently formed in the central of 30 Dor, including the R136 cluster. Using the photometric catalog of De Marchi et al., based on observations with the Hubble Space Telescope, and the most recent ...
G. Marchi, N. Panagia, G. Beccari
semanticscholar   +1 more source

High-precision Dynamical Masses of Pre-main-sequence Stars with ALMA and Gaia [PDF]

open access: yesAstrophysical Journal, 2019
The Keplerian rotation in protoplanetary disks can be used to robustly measure stellar masses at very high precision if the source distance is known. We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of spatially and spectrally ...
P. Sheehan   +3 more
semanticscholar   +1 more source

Pre-main sequence stars in the Lagoon Nebula (M8) [PDF]

open access: yes, 2006
We report the discovery of new pre-main sequence (PMS) stars in the Lagoon Nebula (M8) at a distance of 1.25 kpc, based on intermediate resolution spectra obtained with the Boller & Chivens spectrograph at the 6.5-m Magellan I telescope (Las Campanas ...
Arias   +35 more
core   +4 more sources

A Study of ISO Spectra for Herbig Ae/Be Stars [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2002
We present the infrared spectra of Herbig Ae/Be stars including the Infrared Space Observatory (ISO) data. To investigate the overall properties of their circumstellar dust envelope and/or disk, we combine the IR spectra with photometric data ranging ...
Kyung-Won Suh, Mi-Ryang Kim, Ji-Hye Baek
doaj   +1 more source

Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretion [PDF]

open access: yesAstronomy & Astrophysics, 2019
Grids of stellar models are useful tools to derive the properties of stellar clusters, in particular young clusters hosting massive stars, and to provide information on the star formation process in various mass ranges.
L. Haemmerlé   +8 more
semanticscholar   +1 more source

XUE: Molecular Inventory in the Inner Region of an Extremely Irradiated Protoplanetary Disk

open access: yesThe Astrophysical Journal Letters, 2023
We present the first results of the eXtreme UV Environments (XUE) James Webb Space Telescope (JWST) program, which focuses on the characterization of planet-forming disks in massive star-forming regions.
María Claudia Ramírez-Tannus   +26 more
doaj   +1 more source

Hubble Tarantula Treasury Project - VI. Identification of pre-main-sequence stars using machine-learning techniques [PDF]

open access: yes, 2018
The Hubble Tarantula Treasury Project (HTTP) has provided an unprecedented photometric coverage of the entire star-burst region of 30 Doradus down to the half Solar mass limit.
Victor F. Ksoll   +24 more
semanticscholar   +1 more source

Revisiting the pre-main-sequence evolution of stars [PDF]

open access: yesAstronomy & Astrophysics, 2017
Aims. We want to investigate how planet formation is imprinted on stellar surface composition using up-to-date stellar evolution models. Methods. We simulate the evolution of pre-main-sequence stars as a function of the efficiency of heat injection ...
M. Kunitomo   +3 more
semanticscholar   +1 more source

Long-term optical photometric monitoring of the FUor star V900 Mon [PDF]

open access: yesSerbian Astronomical Journal, 2021
We present results from photometric monitoring of V900 Mon, one of the newly discovered and still under-studied object from the FU Orionis type. The FUor phenomenon is very rarely observed, but it is essential for stellar evolution.
Semkov E.H., Peneva S.P., Ibryamov S.I.
doaj   +1 more source

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