3
... M dwarfs) are fully convective, and are expected to have a different type of dynamo mechanism than...
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4
... to be mid-to-late M dwarfs. We fit an astrometric model to MEarth's images for 1507 stars and obtained...
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5
...We present deep H I 21 cm and optical observations of the face-on spiral galaxy M 83 obtained...
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6
...We report on a year-long effort to monitor the central supermassive black hole in M81 in the X-ray...
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7
... of M31 in generating the high angular momentum orbit of the Clouds, a puzzle that has only been...
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8
... technique. This effect is particularly of concern for M dwarfs, which can remain magnetically active...
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9
by West, Andrew A., Basri, Gibor
Published 2015
...We have examined the relationship between rotation and activity in 14 late-type (M6–M7) M dwarfs...
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10
...The overtone and multi-mode RR Lyrae stars in the globular cluster M3 are studied using a 200 day...
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11
... the literature, our sample comprises 2202 measurements or non-detections of Hα emission in nearby M dwarfs...
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12
...We present an analysis of 15 Chandra observations of the nearby spiral galaxy M81 taken over...
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13
...We present the analysis of two observations of M92 taken with the Chandra X-Ray Observatory. We...
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15
... the spiral galaxy M94. The source has been observed by ROSAT, Chandra, and XMM-Newton on several occasions...
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17
...We study a Chandra X-ray Observatory ACIS-S observation of the Galactic globular cluster M12...
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18
... Telescope Multiband Imaging Photometer 24 μm observations of the previously used X-ray sample, and we find...
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20
...We present a flare rate analysis of 50,130 M dwarf light curves in Sloan Digital Sky Survey Stripe...
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