Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory
We present an analysis of two epochs of ACIS observations of the SA(s)c spiral galaxy NGC 3938 with the Chandra X-ray Observatory. The total exposure time of the observations was 95 ks, with a limiting unabsorbed luminosity of ≈10 ^38 erg s ^−1 assuming a distance of 22 Mpc. A total of 47 discrete m...
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2025-01-01
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| author | Siddhi Raut Eric M. Schlegel Thomas G. Pannuti Brannon W. Jones Jacobo Matallana |
| author_facet | Siddhi Raut Eric M. Schlegel Thomas G. Pannuti Brannon W. Jones Jacobo Matallana |
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| description | We present an analysis of two epochs of ACIS observations of the SA(s)c spiral galaxy NGC 3938 with the Chandra X-ray Observatory. The total exposure time of the observations was 95 ks, with a limiting unabsorbed luminosity of ≈10 ^38 erg s ^−1 assuming a distance of 22 Mpc. A total of 47 discrete merged sources from both epochs were detected at the ≈3 σ level or greater with the D25 radius. We demonstrate that at the time of the Chandra observations the nucleus was not detected. We connect the detected sources to counterparts in other wavebands to the degree possible. Based on the two epochs, we identify three variable sources and an additional two that may have varied between the two observations. We do not formally detect any of the five historical supernovae that have occurred in NGC 3938. The luminosity function of NGC 3938 is compared to a recent compilation of 38 galaxies, and we identify a potentially significant problem with the “known” distance to NGC 3938. Star formation rate and metallicity values are also computed; the star formation rate is highly dependent on the adopted distance. The metallicity appears to lie in the range of 8.2–9.2, consistent with values from other work. We include in an appendix a short discussion of the sources that lie in Chandra’s field of view but lie outside of NGC 3938. |
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| institution | Kabale University |
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| language | English |
| publishDate | 2025-01-01 |
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| spelling | doaj-art-1ba2bbf651cc4d568a39e6410d589a832025-02-03T13:44:17ZengIOP PublishingThe Astronomical Journal1538-38812025-01-01169211010.3847/1538-3881/ad9eb4Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray ObservatorySiddhi Raut0Eric M. Schlegel1https://orcid.org/0000-0002-4162-8190Thomas G. Pannuti2https://orcid.org/0000-0001-7658-1065Brannon W. Jones3Jacobo Matallana4Ronald Reagan High School , 19000 Ronald Reagan, San Antonio, TX 78258, USA ; siddhi.raut.missionartemis@gmail.comDepartment of Physics and Astronomy, University of Texas at San Antonio , One UTSA Circle, San Antonio, TX 78249, USA ; eric.schlegel@utsa.eduDepartment of Engineering Science, 123 Lappin Hall, Morehead State University , 150 University Drive, Morehead, KY 40351, USA ; t.pannuti@moreheadstate.eduDepartment of Engineering Science, 123 Lappin Hall, Morehead State University , 150 University Drive, Morehead, KY 40351, USA ; t.pannuti@moreheadstate.eduDepartment of Engineering Science, 123 Lappin Hall, Morehead State University , 150 University Drive, Morehead, KY 40351, USA ; t.pannuti@moreheadstate.eduWe present an analysis of two epochs of ACIS observations of the SA(s)c spiral galaxy NGC 3938 with the Chandra X-ray Observatory. The total exposure time of the observations was 95 ks, with a limiting unabsorbed luminosity of ≈10 ^38 erg s ^−1 assuming a distance of 22 Mpc. A total of 47 discrete merged sources from both epochs were detected at the ≈3 σ level or greater with the D25 radius. We demonstrate that at the time of the Chandra observations the nucleus was not detected. We connect the detected sources to counterparts in other wavebands to the degree possible. Based on the two epochs, we identify three variable sources and an additional two that may have varied between the two observations. We do not formally detect any of the five historical supernovae that have occurred in NGC 3938. The luminosity function of NGC 3938 is compared to a recent compilation of 38 galaxies, and we identify a potentially significant problem with the “known” distance to NGC 3938. Star formation rate and metallicity values are also computed; the star formation rate is highly dependent on the adopted distance. The metallicity appears to lie in the range of 8.2–9.2, consistent with values from other work. We include in an appendix a short discussion of the sources that lie in Chandra’s field of view but lie outside of NGC 3938.https://doi.org/10.3847/1538-3881/ad9eb4Spiral galaxiesX-ray astronomyX-ray sources |
| spellingShingle | Siddhi Raut Eric M. Schlegel Thomas G. Pannuti Brannon W. Jones Jacobo Matallana Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory The Astronomical Journal Spiral galaxies X-ray astronomy X-ray sources |
| title | Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory |
| title_full | Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory |
| title_fullStr | Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory |
| title_full_unstemmed | Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory |
| title_short | Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory |
| title_sort | multiepoch observations of the nearby spiral galaxy ngc 3938 with the chandra x ray observatory |
| topic | Spiral galaxies X-ray astronomy X-ray sources |
| url | https://doi.org/10.3847/1538-3881/ad9eb4 |
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