Results 41 to 50 of about 5,486 (209)

The OB-type subdwarf HD 149382 and the nature of the subdwarf B stars

open access: yesThe Astrophysical Journal, 1975
High-dispersion spectra and monochromatic continuum measures of the subdwarf OB star HD 149382 have been obtained and analyzed to yield the atmospheric parameters T)=40,000 K, log g=5.8. Helium is deficient by a factor 10 compared to Population I. Sulfur is the only element, other than hydrogen and helium, observed in the blue spectrum of this object ...
B. Baschek, J. Norris
openaire   +1 more source

The discovery of a T6.5 subdwarf [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
We report the discovery of ULAS J131610.28+075553.0, a sdT6.5 dwarf in the UKIDSS Large Area Survey 2 epoch proper motion catalogue. This object displays significant spectral peculiarity, with the largest yet seen deviations from T6 and T7 templates in the Y and K bands for this subtype.
B. Burningham   +6 more
openaire   +2 more sources

Primeval very low-mass stars and brown dwarfs - III. The halo transitional brown dwarfs [PDF]

open access: yes, 2018
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.We report the discovery of an
A J Burgasser   +78 more
core   +6 more sources

Rotation in sdB stars as revealed by stellar oscillations

open access: yesOpen Astronomy, 2018
An interesting opportunity offered by the detection of stellar oscillations is the possibility to infer the internal rotation rate of a star through the so-called rotational splittings. Such seismic measurements remained rather scarce for hot B subdwarf (
Charpinet Stephane   +5 more
doaj   +1 more source

The Unseen Population of F to K-type Companions to Hot Subdwarf Stars

open access: yes, 2012
We present a method to select hot subdwarf stars with A to M-type companions using photometric selection criteria. We cover a wide range in wavelength by combining GALEX ultraviolet data, optical photometry from the SDSS and the Carlsberg Meridian ...
Abazajian   +98 more
core   +1 more source

A small survey of UV-bright stars around the northern ecliptic pole: seeking new p-mode sdB variables for the TESS mission

open access: yesOpen Astronomy, 2019
Starting in 2019, the TESS mission will monitor the northern ecliptic pole for 1 year. Data will be collected at 30-minute and 2-minute cadences, and only a limited amount of slots will be reserved for targets requiring a 20- second cadence.
Prins Saskia   +2 more
doaj   +1 more source

Discoveries from a Near-infrared Proper Motion Survey using Multi-epoch 2MASS Data [PDF]

open access: yes, 2010
We have conducted a 4030-square-deg near-infrared proper motion survey using multi-epoch data from the Two Micron All-Sky Survey (2MASS). We find 2778 proper motion candidates, 647 of which are not listed in SIMBAD.
Adam J. Burgasser   +85 more
core   +3 more sources

Se-ResNet+SVM Model: An Effective Method of Searching for Hot Subdwarfs from LAMOST

open access: yesThe Astrophysical Journal Supplement Series
This paper presents a robust neural network approach for identifying hot subdwarfs. Our method leveraged the Squeeze-and-Excitation Residual Network to extract abstract features, which were combined with experience features to create hybrid features ...
Zhongding Cheng   +9 more
doaj   +1 more source

Spectral energy distributions and colours of hot subluminous stars

open access: yesOpen Astronomy, 2018
Photometric surveys at optical, ultraviolet, and infrared wavelengths provide ever-growing datasets as major surveys proceed. Colour-colour diagrams are useful tools to identify classes of star and provide large samples.
Heber Ulrich   +2 more
doaj   +1 more source

A 500 pc volume-limited sample of hot subluminous stars

open access: yesAstronomy & Astrophysics
We present a quantitative spectroscopic and kinematic analysis of a volume-complete sample of hot subluminous stars within 500 pc of the Sun, assembled using accurate parallax measurements from the Gaia space mission Data Release 3 (DR3).
Dawson H.   +32 more
doaj   +1 more source

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