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<titleInfo><title>Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess</title></titleInfo>


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  <namePart type="given">Lisa</namePart>
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  <namePart type="given">Kareem</namePart>
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  <namePart type="given">Bethany</namePart>
  <namePart type="family">Ludwig</namePart>
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  <namePart type="given">Maria R.</namePart>
  <namePart type="family">Drout</namePart>
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  <namePart type="given">Ylva Louise Linsdotter</namePart>
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<abstract lang="eng">Stripped stars are hot, helium-rich stars formed when binary interactions remove a star’s hydrogen envelope. While low-mass (≲1 M⊙) and high-mass (≳8 M⊙) stripped stars are well studied as hot subdwarfs and Wolf–Rayet stars, their intermediate-mass counterparts (1–8 M⊙) have only recently been discovered. The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS) identified UV-excess sources (i.e., sources lying blueward of the main sequence) in the Magellanic Clouds using Swift-UVOT photometry and selected 820 photometric stripped-star candidates. However, the completeness and purity of this sample remain poorly understood. We forward model the population of stripped stars in the Magellanic Clouds using a binary population synthesis model combined with spatially resolved star formation histories and simulated UV photometry. To assess survey sensitivity, we inject simulated sources into real Swift-UVOT images and reproduce the SUMS selection process, including crowding, extinction, and photometric quality cuts. For the SMC and LMC, we respectively recover 31% and 15% of sources with intrinsic UV excess, and 11% and 7% of all stripped stars. The rest are missed due to dilution by luminous companions, crowding, high extinction, and limited survey coverage. The observed population is biased toward systems with low-mass companions formed by common envelope evolution and systems with compact object companions. We predict contamination of the observed stripped-star candidates by main-sequence stars with spurious UV excess due to crowding and provide guidelines for selecting higher-purity subsamples. Our population synthesis model matches the number and properties of observed stripped star candidates with masses of (2–5) M⊙ well. It underpredicts the number of lower- and higher-mass candidates, perhaps due to contamination.</abstract>

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<originInfo><publisher>IOP Publishing</publisher><dateIssued encoding="w3cdtf">2026</dateIssued>
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<relatedItem type="host"><titleInfo><title>Publications of the Astronomical Society of the Pacific</title></titleInfo>
  <identifier type="issn">0004-6280</identifier>
  <identifier type="eIssn">1538-3873</identifier>
  <identifier type="arXiv">2510.18965</identifier><identifier type="doi">10.1088/1538-3873/ae3a19</identifier>
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<ama>Blomberg L, El-Badry K, Ludwig B, Drout MR, Götberg YLL. Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess. &lt;i&gt;Publications of the Astronomical Society of the Pacific&lt;/i&gt;. 2026;138(2). doi:&lt;a href=&quot;https://doi.org/10.1088/1538-3873/ae3a19&quot;&gt;10.1088/1538-3873/ae3a19&lt;/a&gt;</ama>
<chicago>Blomberg, Lisa, Kareem El-Badry, Bethany Ludwig, Maria R. Drout, and Ylva Louise Linsdotter Götberg. “Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered via UV Excess.” &lt;i&gt;Publications of the Astronomical Society of the Pacific&lt;/i&gt;. IOP Publishing, 2026. &lt;a href=&quot;https://doi.org/10.1088/1538-3873/ae3a19&quot;&gt;https://doi.org/10.1088/1538-3873/ae3a19&lt;/a&gt;.</chicago>
<short>L. Blomberg, K. El-Badry, B. Ludwig, M.R. Drout, Y.L.L. Götberg, Publications of the Astronomical Society of the Pacific 138 (2026).</short>
<ista>Blomberg L, El-Badry K, Ludwig B, Drout MR, Götberg YLL. 2026. Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess. Publications of the Astronomical Society of the Pacific. 138(2), 024202.</ista>
<ieee>L. Blomberg, K. El-Badry, B. Ludwig, M. R. Drout, and Y. L. L. Götberg, “Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess,” &lt;i&gt;Publications of the Astronomical Society of the Pacific&lt;/i&gt;, vol. 138, no. 2. IOP Publishing, 2026.</ieee>
<apa>Blomberg, L., El-Badry, K., Ludwig, B., Drout, M. R., &amp;#38; Götberg, Y. L. L. (2026). Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess. &lt;i&gt;Publications of the Astronomical Society of the Pacific&lt;/i&gt;. IOP Publishing. &lt;a href=&quot;https://doi.org/10.1088/1538-3873/ae3a19&quot;&gt;https://doi.org/10.1088/1538-3873/ae3a19&lt;/a&gt;</apa>
<mla>Blomberg, Lisa, et al. “Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered via UV Excess.” &lt;i&gt;Publications of the Astronomical Society of the Pacific&lt;/i&gt;, vol. 138, no. 2, 024202, IOP Publishing, 2026, doi:&lt;a href=&quot;https://doi.org/10.1088/1538-3873/ae3a19&quot;&gt;10.1088/1538-3873/ae3a19&lt;/a&gt;.</mla>
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