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19972025
most citedThe Revised TESS Input Catalog and Candidate Target List

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11 papers · 1 filter

astro-ph2007★ 36 cited

An Extremely Bright Echo Associated With SN 2002hh

D. L. Welch, Geoffrey C. Clayton, Amy Campbell +4

We present new, very late-time optical photometry and spectroscopy of the interesting Type II-P supernova, SN 2002hh, in NGC 6946. Gemini/GMOS-N has been used to acquire visible sp…

astro-ph2006★ 69 cited

V605 Aql: The Older Twin of Sakurai's Object

Geoffrey C. Clayton, F. Kerber, N. Pirzkal +3

New optical spectra have been obtained with VLT/FORS2 of the final helium shell flash (FF) star, V605 Aql, which peaked in brightness in 1919. New models suggest that this star is…

astro-ph2005★ 34 cited

Discovery of Five New R Coronae Borealis Stars in the MACHO Galactic Bulge Database

A. Zaniewski, Geoffrey C. Clayton, D. L. Welch +3

We have identified five new R Coronae Borealis (RCB) stars in the Galactic bulge using the MACHO Project photometry database, raising the total number of known Galactic RCB stars t…

astro-ph2005★ 2 cited

A Unique Dust Formation Episode in the SC-Type Star UY Cen

Justin D. R. Steinfadt, Geoffrey C. Clayton, Tom Lloyd Evans +1

We report the first detection of new dust formation in an SC star. The prototype of the SC stars, UY Cen, underwent a decline of 2 magnitudes in the V-band. The SC stars show pulsa…

astro-ph2005★ 9 cited

Detection of Near-IR CO Absorption Bands in R Coronae Borealis Stars

Emily D. Tenenbaum, Geoffrey C. Clayton, Martin Asplund +8

R Coronae Borealis (RCB) stars are hydrogen-deficient, carbon-rich pulsating post-AGB stars that experience massive irregular declines in brightness caused by circumstellar dust fo…

astro-ph2005★ 45 cited

An Extremely Large Excess of 18O in the Hydrogen-Deficient Carbon Star, HD 137613

Geoffrey C. Clayton, Falk Herwig, T. R. Geballe +4

We report the discovery of a uniquely large excess of 18O in the hydrogen-deficient carbon (HdC) star, HD 137613, based on a spectrum of the first overtone bands of CO at 2.3-2.4 m…