The 40 pc sample of white dwarfs from Gaia
MW O'Brien, PE Tremblay, BL Klein… - Monthly Notices of …, 2024 - academic.oup.com
We present a comprehensive overview of a volume-complete sample of white dwarfs
located within 40 pc of the Sun, a significant proportion of which were detected in Gaia Data …
located within 40 pc of the Sun, a significant proportion of which were detected in Gaia Data …
Cool subdwarf investigations. I. New thoughts on the spectral types of K and M subdwarfs
WC Jao, TJ Henry, TD Beaulieu… - The Astronomical …, 2008 - iopscience.iop.org
Using new spectra of 88 K-and M-type subdwarfs, we consider novel methods for assigning
their spectral types and take steps toward developing a comprehensive spectral sequence …
their spectral types and take steps toward developing a comprehensive spectral sequence …
Wolf 1130: A Nearby Triple System Containing a Cool, Ultramassive White Dwarf
GN Mace, AW Mann, BA Skiff, C Sneden… - The Astrophysical …, 2018 - iopscience.iop.org
Following the discovery of the T8 subdwarf WISE J200520. 38+ 542433.9 (Wolf 1130C),
which has a proper motion in common with a binary (Wolf 1130AB) consisting of an M …
which has a proper motion in common with a binary (Wolf 1130AB) consisting of an M …
A new sample of cool subdwarfs from SDSS: properties and kinematics
AS Savcheva, AA West… - The Astrophysical Journal, 2014 - iopscience.iop.org
We present a new sample of M subdwarfs compiled from the seventh data release of the
Sloan Digital Sky Survey. With 3517 new subdwarfs, this new sample significantly increases …
Sloan Digital Sky Survey. With 3517 new subdwarfs, this new sample significantly increases …
The chromospheric activity, age, metallicity, and space motions of 36 wide binaries
We present the chromospheric activity (CA) levels, metallicities, and full space motions for
41 F, G, K, and M dwarf stars in 36 wide binary systems. Thirty-one of the binaries contain a …
41 F, G, K, and M dwarf stars in 36 wide binary systems. Thirty-one of the binaries contain a …
A spectroscopic and proper motion search of Sloan Digital Sky Survey: red subdwarfs in binary systems
ZH Zhang, DJ Pinfield, B Burningham… - Monthly Notices of …, 2013 - academic.oup.com
Red subdwarfs in binary systems are crucial for both model calibration and spectral
classification. We search for red subdwarfs in binary systems from a sample of high proper …
classification. We search for red subdwarfs in binary systems from a sample of high proper …
Mapping the Local Halo: Statistical Parallax Analysis of SDSS Low-mass Subdwarfs
JJ Bochanski, A Savcheva, AA West… - The Astronomical …, 2013 - iopscience.iop.org
We present a statistical parallax study of nearly 2000 M subdwarfs with photometry and
spectroscopy from the Sloan Digital Sky Survey (SDSS). Statistical parallax analysis yields …
spectroscopy from the Sloan Digital Sky Survey (SDSS). Statistical parallax analysis yields …
The DODO survey–II. A Gemini direct imaging search for substellar and planetary mass companions around nearby equatorial and Northern hemisphere white dwarfs
E Hogan, MR Burleigh, FJ Clarke - Monthly Notices of the Royal …, 2009 - academic.oup.com
The aim of the Degenerate Objects around Degenerate Objects (DODO) survey is to search
for very low-mass brown dwarfs and extrasolar planets in wide orbits around white dwarfs …
for very low-mass brown dwarfs and extrasolar planets in wide orbits around white dwarfs …
The Solar Neighborhood. XLII. Parallax results from the CTIOPI 0.9 m program—identifying new nearby subdwarfs using tangential velocities and locations on the H …
WC Jao, TJ Henry, JG Winters… - The Astronomical …, 2017 - iopscience.iop.org
Parallaxes, proper motions, and optical photometry are presented for 51 systems consisting
of 37 cool subdwarf and 14 additional high proper motion systems. Thirty-seven systems …
of 37 cool subdwarf and 14 additional high proper motion systems. Thirty-seven systems …
First discovery of an ultra-cool white dwarf benchmark in common proper motion with an M dwarf
Ultra-cool white dwarfs are among the oldest stellar remnants in the Universe. Their efficient
gravitational settling and low effective temperatures are responsible for the smooth spectra …
gravitational settling and low effective temperatures are responsible for the smooth spectra …