activity
20122026
most citedALMA observations of the Corvi debris disc: inward scattering of CO-rich exocomets by a chain of 3-30 M planets?

103 citations · 241 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2026

Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation

Emma V. Turtelboom, Steven Giacalone, Rebecca Gore +6

M dwarfs are the most common sites of planet formation in the Milky Way. Planet occurrence and composition are closely linked with the availability of metals in protoplanetary disk…

astro-ph.SR2025

First Resolution of a Main Sequence G-Star Astrosphere Using Chandra

C. M. Lisse, S. J. Wolk, B. Snios +24

We report resolution of a halo of X-ray line emission surrounding the Zero Age Main Sequence (ZAMS) G8.5V star HD 61005 by Chandra ACIS-S. Located only 36.4 pc distant, HD 61005 is…

astro-ph.GA2025★ 2 cited

The Lyman alpha Sky as Observed by New Horizons

G. R. Gladstone, J. M. Shull, W. R. Pryor +22

During September 2023 the Alice ultraviolet spectrograph on the New Horizons (NH) spacecraft was used to map diffuse Lyman alpha (Lya) emission over most of the sky, at a range of…

astro-ph.SR2024★ 14 cited

X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates

K. G. Kislyakova, M. Güdel, D. Koutroumpa +3

Stellar winds of cool main sequence stars are very difficult to constrain observationally. One way to measure stellar mass loss rates is to detect soft X-ray emission from stellar…

astro-ph.IM2023★ 7 cited

Synergies between interstellar dust and heliospheric science with an Interstellar Probe

Veerle J. Sterken, Silvan Hunziker, Kostas Dialynas +40

We discuss the synergies between heliospheric and dust science, the open science questions, the technological endeavors and programmatic aspects that are important to maintain or d…

astro-ph.EP2022★ 14 cited

Mid-infrared spectra of differentiated meteorites (achondrites): Comparison with astronomical observations of dust in protoplanetary and debris disks

A. Morlok, C. Koike, K. Tomeoka +4

Mid-infrared (5 micron to 25 micron) transmission/absorption spectra of differentiated meteorites (achondrites) were measured to permit comparison with astronomical observations of…

astro-ph.SR2017★ 14 cited

Spectral Evidence for an Inner Carbon-Rich Circumstellar Dust Belt in the Young HD36546 A-Star System

Carey M. Lisse, Mike L. Sitko, Ray W. Russell +5

Using the NASA/IRTF SpeX & BASS spectrometers we have obtained novel 0.7 - 13 um observations of the newly imaged HD36546 debris disk system. The SpeX spectrum is most consistent w…

astro-ph.EP2016★ 103 cited

ALMA observations of the Corvi debris disc: inward scattering of CO-rich exocomets by a chain of 3-30 M planets?

S. Marino, M. C. Wyatt, O. Panic +10

While most of the known debris discs present cold dust at tens of AU, a few young systems exhibit hot dust analogous to the Zodiacal dust. Corvi is particularly interesting as…

astro-ph.EP2016★ 26 cited

The Puzzling Detection of X-rays From Pluto by Chandra

C. M. Lisse, R. L. McNutt, S. J. Wolk +17

Using Chandra ACIS-S, we have obtained imaging Xray spectrophotometry of the Pluto system in support of the New Horizons flyby on 14 July 2015. 174 ksec of observations were obtain…

astro-ph.EP2015★ 22 cited

Solar Wind at 33 AU: Setting Bounds on the Pluto Interaction for New Horizons

F. Bagenal, P. A. Delamere, H. A. Elliott +7

The NASA New Horizons spacecraft flies past Pluto on July 14, 2015, carrying two instruments that detect charged particles. Pluto has a tenuous, extended atmosphere that is escapin…

astro-ph.EP2013★ 19 cited

Evolution from protoplanetary to debris discs: The transition disc around HD 166191

G. M. Kennedy, S. J. Murphy, C. M. Lisse +12

HD 166191 has been identified by several studies as hosting a rare and extremely bright warm debris disc with an additional outer cool disc component. However, an alternative inter…

astro-ph.SR2012★ 20 cited

Soft coronal X-rays from β Pictoris

H. M. Günther, S. J. Wolk, J. J. Drake +3

A type stars are expected to be X-ray dark, yet weak emission has been detected from several objects in this class. We present new Chandra/HRC-I observations of the A5 V star β Pic…