Searching for New Supernova Remnant Candidates from the VTSS Survey

Elif Beklen

doi:10.17776/csj.1188709

EN

Searching for New Supernova Remnant Candidates from the VTSS Survey

Abstract

The Virginia Tech Spectral Line Survey (VTSS) Galactic Plane Hydrogen-Alpha Survey has the strong ability to search and discover many different types of objects that cannot be identified clearly on red plates and by other Multi-Wavelength Sky Surveys. Here we make a visual search from the VTSS fields with the supportive surveys of Southern Hydrogen-Alpha Sky Survey Atlas (SHASSA) and MDW Hydrogen-Alpha Sky Survey (MDWS) fields, in the Galactic latitude of |b| between -17 ° and 7 ° for several new optical emission nebulae. Seven candidates were chosen as most likely supernova remnant candidates by their physical shapes and the three of all having [SII]/Hα ratio larger than 0.4, found with T100 photometric observations, are considered to be supernova remnant candidates. Comprehensive optical imaging and spectroscopic observations with multi-wavelength observations will help us to identify the types of all these galactic candidates, more precisely.

Keywords

surveys, ISM: supernova remnants, Optical

Supporting Institution

TÜBİTAK National Observatory - Gözlemevi (TUG)

Project Number

18AT100-1309

Thanks

I would like to thank TUBITAK National Observatory for a partial support in using T100 telescope with project number 18AT100-1309. Also, I would like to thank the Virginia Tech Spectral-Line Survey (VTSS), which is supported by the National Science Foundation. This work made use of Astropy a community-developed core Python package and an ecosystem of tools and resources for astronomy.

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Details

Primary Language

English

Subjects

Classical Physics (Other)

Journal Section

Research Article

Authors

Elif Beklen ^*
0000-0002-4807-2180
Türkiye

Publication Date

December 27, 2022

Submission Date

October 13, 2022

Acceptance Date

December 7, 2022

Published in Issue

Year 2022 Volume: 43 Number: 4

DOI

https://doi.org/10.17776/csj.1188709

IZ

https://izlik.org/JA98FY99WD

APA

Beklen, E. (2022). Searching for New Supernova Remnant Candidates from the VTSS Survey. Cumhuriyet Science Journal, 43(4), 760-768. https://doi.org/10.17776/csj.1188709

AMA

1.Beklen E. Searching for New Supernova Remnant Candidates from the VTSS Survey. CSJ. 2022;43(4):760-768. doi:10.17776/csj.1188709

Chicago

Beklen, Elif. 2022. “Searching for New Supernova Remnant Candidates from the VTSS Survey”. Cumhuriyet Science Journal 43 (4): 760-68. https://doi.org/10.17776/csj.1188709.

EndNote

Beklen E (December 1, 2022) Searching for New Supernova Remnant Candidates from the VTSS Survey. Cumhuriyet Science Journal 43 4 760–768.

IEEE

[1]E. Beklen, “Searching for New Supernova Remnant Candidates from the VTSS Survey”, CSJ, vol. 43, no. 4, pp. 760–768, Dec. 2022, doi: 10.17776/csj.1188709.

ISNAD

Beklen, Elif. “Searching for New Supernova Remnant Candidates from the VTSS Survey”. Cumhuriyet Science Journal 43/4 (December 1, 2022): 760-768. https://doi.org/10.17776/csj.1188709.

JAMA

1.Beklen E. Searching for New Supernova Remnant Candidates from the VTSS Survey. CSJ. 2022;43:760–768.

MLA

Beklen, Elif. “Searching for New Supernova Remnant Candidates from the VTSS Survey”. Cumhuriyet Science Journal, vol. 43, no. 4, Dec. 2022, pp. 760-8, doi:10.17776/csj.1188709.

Vancouver

1.Elif Beklen. Searching for New Supernova Remnant Candidates from the VTSS Survey. CSJ. 2022 Dec. 1;43(4):760-8. doi:10.17776/csj.1188709

As of 2026, Cumhuriyet Science Journal will be published in six issues per year, released in February, April, June, August, October, and December

Abstract

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Searching for New Supernova Remnant Candidates from the VTSS Survey

Abstract

Keywords

Supporting Institution

Project Number

Thanks

References

Details

Primary Language

Subjects

Journal Section

Authors

Publication Date

Submission Date

Acceptance Date

Published in Issue

DOI

IZ

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