The planet's radius is very unusual as M -
dwarf field stars rarely have Neptune - sized transiting planets.
Not exact matches
The three bands then correspond to the galactic center of a galaxy in the Hubble
field and the interacting galaxy, the center of a bright
star in the Magellanic cloud and a
star cluster and the last band corresponds to the white
dwarf in the Helix and Cat's eye nebulae.
As general relativity predicts, light from the background
star bent around the white
dwarf, distorted by its gravitational
field.
A «brown
dwarf»
star that appears to be the coldest of its kind — as frosty as Earth's North Pole — has been discovered by a Penn State University astronomer using NASA's Wide -
field Infrared Survey Explorer (WISE) and Spitzer Space Telescopes.
Previous ground - based observations characterized all the possible targets in each
field (Deleuil et al. 2009); during the target selection, this allowed preference to be given to likely
dwarf stars and hence to maximize the probability of finding a transiting planet.
That change caused the minor planet to travel very close to the white
dwarf, where the
star's strong gravitational
field ripped the minor planet apart into gas and dust.
But if this active magnetic region is long - lasting and representative of its global magnetic
field, LSR J1835 +3259 is way more «
star - like» than we give brown
dwarfs credit for.
We identify PSO J060.3200 +25.9644 (near - infrared spectral type L1) and PSO J077.1033 +24.3809 (L2) as new members of Taurus based on... ▽ More We present the discovery of eight young M7 - L2
dwarfs in the Taurus
star - forming region and the Scorpius - Centaurus OB Association, serendipitously found during a wide -
field search for L / T transition
dwarfs using Pan-STARRS1 (optical) and WISE (mid-infrared) photometry.
It implies that reliable ages can be derived for
field dwarf stars with measured colors and rotation periods, and it promises to enable further understanding of various aspects of stellar rotation and activity for cool
stars.
The type of radio emission seen in the brown
dwarfs arises in more - massive
stars as a result of plasma interacting with the
star's magnetic
field.
Field image around GJ 1214, a very dim, red
dwarf star not visible with the naked eye (more).
I am characterizing the magnetic
fields of ultra-cool brown
dwarf stars in an effort to understand the magnetic dynamo mechanisms operating in the mass regime that bridges planets and
stars.