Araştırma Makalesi
BibTex RIS Kaynak Göster

Searching for New Supernova Remnant Candidates from the VTSS Survey

Yıl 2022, Cilt: 43 Sayı: 4, 760 - 768, 27.12.2022

Elif Beklen

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

Öz

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.

Anahtar Kelimeler

surveys ISM: supernova remnants Optical

Destekleyen Kurum

TÜBİTAK National Observatory - Gözlemevi (TUG)

Proje Numarası

18AT100-1309

Teşekkür

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.

Kaynakça

  • [1] Green D.A., A revised catalogue of 294 Galactic supernova remnants, J. Astrophys. Astr., 40 (4) (2019) 36-48.
  • [2] Downes D., New Radio Results on Supernova Remnants, AJ, 76 (1971) 305-316.
  • [3] Chevalier R.A., The interaction of supernovae with the interstellar medium, ARAA, 15 (1977) 175-196.
  • [4] Kopsacheili M., Zezas A., Leonidaki I., A diagnostic tool for the identification of supernova remnants, MNRAS, 491 (2020) 889-902.
  • [5] Boumis P., Xilouris E. M., Alikakos J., Christopoulou,P. E., Mavromatakis F, Katsiyannis A. C., Goudis C. D., Discovery of optical emission from the supernova remnant G 32.8-0.1 (Kes 78), A&A, 499 (3) (2009) 789-797.
  • [6] Stupar, M., Parker Q. A., Optical detection and spectroscopic confirmation of supernova remnant G213.0-0.6 (now redesignated as G213.3-0.4), MNRAS, 419 (2) (2012) 1413-1420.
  • [7] Neustadt J. M. M., Fesen R. A., Black C. S., Detection of optical emission associated with the Galactic SNR G64.5+0.9, MNRAS, 469 (2017) 516-520.
  • [8] Stupar M., Parker Q. A., Frew D. J., Confirmation of G6.31+0.54 as a part of a Galactic supernova remnant, MNRAS, 479 (2018) 4432-4439.
  • [9] How T. G., Fesen R. A., Neustadt J. M. M., Black C. S., Outter, N., Optical emission associated with the Galactic supernova remnant G179.0+2.6, MNRAS, 478 (2) (2018) 1987-1993.
  • [10] Fesen R. A., Neustadt J. M. M., How T. G., Black C. S., Detection of extensive optical emission from the extremely radio faint Galactic supernova remnant G182.4+4.3, MNRAS, 486 (4) (2019) 4701- 4709.
  • [11] Fesen R.A., Weil K. E., Raymond J.C., Huet L., Rusterholz M., Di Cicco D., Mittelman D., Walker S., Drechsler M. and Faworski S., G107.0+9.0: a new large optically bright, radio, and X-Ray faint galactic supernova remnant in Cepheus, MNRAS, 498 (4) (2020) 5194–5206.
  • [12] Fesen R.A., Neustadt J.M.M., Black C.S. and Koeppel. A.H.D., Discovery of an Apparent High Latitude Galactic Supernova Remnant, AJ, 812 (1) (2015) 37-48.
  • [13] Stupar M., Parker Q. A., Filipovic M. D., Newly confirmed and candidate Galactic SNRs uncovered from the AAO/UKST Hα survey, MNRAS, 390 (3) (2008) 1037-1054.
  • [14] Fesen R. A., Milisavljevic D., Optical Discovery of an Apparent Galactic Supernova Remnant G159.6+7.3, AJ, 140 (5) (2010) 1163-1167.
  • [15] Sabin L., Parker Q. A., Contreras M. E., Olguín L., Frew D. J., Stupar M., Vázquez R., Wright N. J., Corradi R. L. M., Morris R. A. H., New Galactic supernova remnants discovered with IPHAS, MNRAS, 431 (1) (2013) 279-291.
  • [16] Dennison B., Simonetti J. H., Topasna G. A., An imaging survey of northern galactic Hα emmission with arcminute resolution, PASA, 15 (1) (1998) 147-148.
  • [17] Finkbeiner D.P., A Full-Sky Hα Template for Microwave Foreground Prediction, ApJS, 146 (2) (2003) 407-415.
  • [18] [Gaustad J. E., McCullough P. R., Rosing W., and Buren D. Van, A Robotic Wide-Angle Hα Survey of the Southern Sky, PASP, 113 (789) (2001) 1326–1348.
  • [19] Drew J.E., Greimel R., Irwin M.J., et al., The INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS), MNRAS, 362 (3) (2005) 753-776.
  • [20] González-Solares E.A., Walton N.A, Greimel R., et al., Initial data release from the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS), MNRAS, 388 (1) (2008) 89-104.
  • [21] Mathewson, D. S., Clarke, J. N., Supernova Remnants in the Magellanic Clouds, AJ, 182 (1973) 697-698.
  • [22] Blair W. P., Kirshner R. P., Chevalier R. A., Supernova remants in M31, ApJ, 247 (1981) 879-893.
  • [23] Dopita M.A., Benvenuti P., Dodorico S., Binette L., Radiative shock-wave theory. I. Chemical abundance diagnostics and galactic abundance gradients, ApJ, 276 (1984) 653-666.
  • [24] Fesen R. A., Blair W. P., Kirshner R. P., Optical emission-line properties of evolved galactic supernova remnants, AJ, 292 (1985) 29-48.
  • [25] Leonidaki I., Boumis P., Zezas A., A multiwavelength study of supernova remnants in six nearby galaxies - II. New optically selected supernova remnants, MNRAS, 429 (1) (2013) 189-220.
  • [26]Long K. S., Galactic and Extragalactic Samples of Supernova Remnants: How They Are Identified and What They Tell Us, in Alsabti A. W., Murdin P., eds, Handbook of Supernovae, Springer International Publishing AG, (2017) 2005-2040.
  • [27] https://doi.org/10.1007/978-3-319-21846-5_90
  • [28]Frew D.J., Bojicic I.S., Parker Q.A., A catalogue of integrated Hα fluxes for 1258 Galactic planetary nebulae, MNRAS, 431 (1) (2013) 2–26.
  • [29]Dharmawardena T. E., Barlow M. J., Drew J. E., Seales A., Sale S. E., Jones D., Mampaso A., Parker Q. A., Sabin L., Wesson R., Hα fluxes and extinction distances for planetary nebulae in the IPHAS survey of the northern galactic plane, MNRAS, 501 (4) (2021) 6156–6167.
  • [30]Anderson L.D., Bania T.M., Balser D. S., Cunningham V., Wenger T. V., Johnstone B.M., and Armentrout W.P., The WISE Catalog of Galactic H II Regions, ApJS, 212 (1) (2014) 1–18.
  • [31] The Astropy Collaboration, Astropy: A community-developed core Python package and an ecosystem of tools and resources for astronomy, AA, 558 (2013) A33.
  • [32]The Astropy Collaboration, Astropy: A community-developed core Python package and an ecosystem of tools and resources for astronomy, AJ, 156 (2018) 123.

Yıl 2022, Cilt: 43 Sayı: 4, 760 - 768, 27.12.2022

Elif Beklen

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

Öz

Proje Numarası

18AT100-1309

Kaynakça

  • [1] Green D.A., A revised catalogue of 294 Galactic supernova remnants, J. Astrophys. Astr., 40 (4) (2019) 36-48.
  • [2] Downes D., New Radio Results on Supernova Remnants, AJ, 76 (1971) 305-316.
  • [3] Chevalier R.A., The interaction of supernovae with the interstellar medium, ARAA, 15 (1977) 175-196.
  • [4] Kopsacheili M., Zezas A., Leonidaki I., A diagnostic tool for the identification of supernova remnants, MNRAS, 491 (2020) 889-902.
  • [5] Boumis P., Xilouris E. M., Alikakos J., Christopoulou,P. E., Mavromatakis F, Katsiyannis A. C., Goudis C. D., Discovery of optical emission from the supernova remnant G 32.8-0.1 (Kes 78), A&A, 499 (3) (2009) 789-797.
  • [6] Stupar, M., Parker Q. A., Optical detection and spectroscopic confirmation of supernova remnant G213.0-0.6 (now redesignated as G213.3-0.4), MNRAS, 419 (2) (2012) 1413-1420.
  • [7] Neustadt J. M. M., Fesen R. A., Black C. S., Detection of optical emission associated with the Galactic SNR G64.5+0.9, MNRAS, 469 (2017) 516-520.
  • [8] Stupar M., Parker Q. A., Frew D. J., Confirmation of G6.31+0.54 as a part of a Galactic supernova remnant, MNRAS, 479 (2018) 4432-4439.
  • [9] How T. G., Fesen R. A., Neustadt J. M. M., Black C. S., Outter, N., Optical emission associated with the Galactic supernova remnant G179.0+2.6, MNRAS, 478 (2) (2018) 1987-1993.
  • [10] Fesen R. A., Neustadt J. M. M., How T. G., Black C. S., Detection of extensive optical emission from the extremely radio faint Galactic supernova remnant G182.4+4.3, MNRAS, 486 (4) (2019) 4701- 4709.
  • [11] Fesen R.A., Weil K. E., Raymond J.C., Huet L., Rusterholz M., Di Cicco D., Mittelman D., Walker S., Drechsler M. and Faworski S., G107.0+9.0: a new large optically bright, radio, and X-Ray faint galactic supernova remnant in Cepheus, MNRAS, 498 (4) (2020) 5194–5206.
  • [12] Fesen R.A., Neustadt J.M.M., Black C.S. and Koeppel. A.H.D., Discovery of an Apparent High Latitude Galactic Supernova Remnant, AJ, 812 (1) (2015) 37-48.
  • [13] Stupar M., Parker Q. A., Filipovic M. D., Newly confirmed and candidate Galactic SNRs uncovered from the AAO/UKST Hα survey, MNRAS, 390 (3) (2008) 1037-1054.
  • [14] Fesen R. A., Milisavljevic D., Optical Discovery of an Apparent Galactic Supernova Remnant G159.6+7.3, AJ, 140 (5) (2010) 1163-1167.
  • [15] Sabin L., Parker Q. A., Contreras M. E., Olguín L., Frew D. J., Stupar M., Vázquez R., Wright N. J., Corradi R. L. M., Morris R. A. H., New Galactic supernova remnants discovered with IPHAS, MNRAS, 431 (1) (2013) 279-291.
  • [16] Dennison B., Simonetti J. H., Topasna G. A., An imaging survey of northern galactic Hα emmission with arcminute resolution, PASA, 15 (1) (1998) 147-148.
  • [17] Finkbeiner D.P., A Full-Sky Hα Template for Microwave Foreground Prediction, ApJS, 146 (2) (2003) 407-415.
  • [18] [Gaustad J. E., McCullough P. R., Rosing W., and Buren D. Van, A Robotic Wide-Angle Hα Survey of the Southern Sky, PASP, 113 (789) (2001) 1326–1348.
  • [19] Drew J.E., Greimel R., Irwin M.J., et al., The INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS), MNRAS, 362 (3) (2005) 753-776.
  • [20] González-Solares E.A., Walton N.A, Greimel R., et al., Initial data release from the INT Photometric Hα Survey of the Northern Galactic Plane (IPHAS), MNRAS, 388 (1) (2008) 89-104.
  • [21] Mathewson, D. S., Clarke, J. N., Supernova Remnants in the Magellanic Clouds, AJ, 182 (1973) 697-698.
  • [22] Blair W. P., Kirshner R. P., Chevalier R. A., Supernova remants in M31, ApJ, 247 (1981) 879-893.
  • [23] Dopita M.A., Benvenuti P., Dodorico S., Binette L., Radiative shock-wave theory. I. Chemical abundance diagnostics and galactic abundance gradients, ApJ, 276 (1984) 653-666.
  • [24] Fesen R. A., Blair W. P., Kirshner R. P., Optical emission-line properties of evolved galactic supernova remnants, AJ, 292 (1985) 29-48.
  • [25] Leonidaki I., Boumis P., Zezas A., A multiwavelength study of supernova remnants in six nearby galaxies - II. New optically selected supernova remnants, MNRAS, 429 (1) (2013) 189-220.
  • [26]Long K. S., Galactic and Extragalactic Samples of Supernova Remnants: How They Are Identified and What They Tell Us, in Alsabti A. W., Murdin P., eds, Handbook of Supernovae, Springer International Publishing AG, (2017) 2005-2040.
  • [27] https://doi.org/10.1007/978-3-319-21846-5_90
  • [28]Frew D.J., Bojicic I.S., Parker Q.A., A catalogue of integrated Hα fluxes for 1258 Galactic planetary nebulae, MNRAS, 431 (1) (2013) 2–26.
  • [29]Dharmawardena T. E., Barlow M. J., Drew J. E., Seales A., Sale S. E., Jones D., Mampaso A., Parker Q. A., Sabin L., Wesson R., Hα fluxes and extinction distances for planetary nebulae in the IPHAS survey of the northern galactic plane, MNRAS, 501 (4) (2021) 6156–6167.
  • [30]Anderson L.D., Bania T.M., Balser D. S., Cunningham V., Wenger T. V., Johnstone B.M., and Armentrout W.P., The WISE Catalog of Galactic H II Regions, ApJS, 212 (1) (2014) 1–18.
  • [31] The Astropy Collaboration, Astropy: A community-developed core Python package and an ecosystem of tools and resources for astronomy, AA, 558 (2013) A33.
  • [32]The Astropy Collaboration, Astropy: A community-developed core Python package and an ecosystem of tools and resources for astronomy, AJ, 156 (2018) 123.
Toplam 32 adet kaynakça vardır.

Ayrıntılar

Birincil Dil İngilizce
Konular Klasik Fizik (Diğer)
Bölüm Natural Sciences
Yazarlar

Elif Beklen 0000-0002-4807-2180

Proje Numarası 18AT100-1309
Yayımlanma Tarihi 27 Aralık 2022
Gönderilme Tarihi 13 Ekim 2022
Kabul Tarihi 7 Aralık 2022
Yayımlandığı Sayı Yıl 2022Cilt: 43 Sayı: 4

Kaynak Göster

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
 Kapak Resmi İndir