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Ruprecht 147

When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147
FY13 High-Level Deliverables
Characterising Open Clusters in the Solar Neighbourhood with the Tycho-Gaia Astrometric Solution? T
Andrew Vanderburg 77 Massachusetts Avenue • Mcnair Building (MIT Building 37) • Cambridge, MA 02139 [email protected] •
Institute of Space Sciences Annual Report 2017
Touchstone Stars: Highlights from the Cool Stars 18 Splinter Session
A Sub-Neptune Exoplanet Transiting a Solar Twin in Ruprecht 147
Proceedings of the 18Th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
K2-231 B: a Sub-Neptune Exoplanet Transiting a Solar Twin in Ruprecht 147
250+ Deep-Sky Objects Visible with 7X35 Binoculars and the Naked-Eye
SCYON Issue 70
$The Putative Old, Nearby Cluster Lod\'{E} N 1 Does Not Exist$

The Putative Old, Nearby Cluster Lod\'{E} N 1 Does Not Exist
Massive White Dwarfs in Young Star Clusters
CCD UBV RI Photometry of the Open Cluster Berkeley 8
Arxiv:2010.02272V1 [Astro-Ph.SR] 5 Oct 2020 Orsodn Uhr Ao E Curtis Lee Jason Author: Corresponding 12 Dml Kraus L
Arxiv:1911.07075V1 [Astro-Ph.SR] 16 Nov 2019
2013 CFHT Annual Report
Arxiv:2103.01747V1 [Astro-Ph.SR] 2 Mar 2021 More Thoroughly Than Most Other Work Has Done

Top View

Open Cluster Kinematics with Gaia DR2? C
Clusters and Mirages: Cataloguing Stellar Aggregates in the Milky Way? T
Arxiv:1901.04253V1 [Astro-Ph.GA] 14 Jan 2019 Produce Mass Functions (MF) Peaked Close to High Mass Stars
Carbon Star Formation As Seen Through the Non-Monotonic Initial-Final Mass Relation
Open Cluster Kinematics with Gaia DR2 C

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