Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Articles Article Faculty Publications -Articles Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource A census of young stellar population associated with the Herbig Be star HD 200775 Subject The topic of the resource ISM: clouds; polarization; stars: distances; stars: pre-main-sequence; X-rays: stars Description An account of the resource The region surrounding the well-known reflection nebula, NGC 7023, illuminated by a Herbig Be star, HD 200775, located in the dark cloud L1174 is studied in this work. Based on the distances and proper motion values from Gaia DR2 of 20 previously known young stellar object (YSO) candidates, we obtained a distance of 335 11 pc to the cloud complex L1172/1174. Using polarization measurements of the stars projected on the cloud complex, we show additional evidence for the cloud to be at ?335 pc distance. Using this distance and proper motion values of the YSO candidates, we searched for additional comoving sources in the vicinity of HD 200775 and found 20 new sources, which show low infrared excess emission and are of age ?1 Myr. Among these, 10 YSO candidates and 4 newly identified comoving sources are found to show X-ray emission. Three of the four new sources for which we have obtained optical spectra show H ? in emission. About 80 per cent of the total sources are found within ?1 pc distance from HD 200775. Spatial correlation of some of the YSO candidates with the Herschel dust column density peaks suggests that star formation is still active in the region and may have been triggered by HD 200775. 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. Creator An entity primarily responsible for making the resource Saha P.; Gopinathan M.; Kamath U.; Lee C.W.; Puravankara M.; Mathew B.; Sharma E. Source A related resource from which the described resource is derived Monthly Notices of the Royal Astronomical Society, Vol-494, No. 4, pp. 5851-5871. Publisher An entity responsible for making the resource available Oxford University Press Date A point or period of time associated with an event in the lifecycle of the resource 2020-01-01 Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.1093/mnras/staa1053" target="_blank" rel="noreferrer noopener">https://doi.org/10.1093/mnras/staa1053</a> <br /><br /><a href="https://www.scopus.com/inward/record.uri?eid=2-s2.0-85096954636&amp;doi=10.1093%2Fmnras%2Fstaa1053&amp;partnerID=40&amp;md5=2b7f174fef612b50fbefeb992b3eff5c" target="_blank" rel="noreferrer noopener">https://www.scopus.com/inward/record.uri?eid=2-s2.0-85096954636&amp;doi=10.1093%2fmnras%2fstaa1053&amp;partnerID=40&amp;md5=2b7f174fef612b50fbefeb992b3eff5c</a> Rights Information about rights held in and over the resource All Open Access; Green Open Access Relation A related resource ISSN: 358711; CODEN: MNRAA Format The file format, physical medium, or dimensions of the resource Online Language A language of the resource English Type The nature or genre of the resource Article Coverage The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant Saha P., Indian Institute of Astrophysics (IIA), Sarjapur Road, Koramangala, Bangalore, Karnataka, 560034, India, Pt. Ravishankar Shukla University, Amanaka G.E. Road, Raipur, Chhatisgarh, 492010, India; Gopinathan M., Indian Institute of Astrophysics (IIA), Sarjapur Road, Koramangala, Bangalore, Karnataka, 560034, India; Kamath U., Indian Institute of Astrophysics (IIA), Sarjapur Road, Koramangala, Bangalore, Karnataka, 560034, India; Lee C.W., Korea Astronomy and Space Science Institute (KASI), 776 Daedeok-daero, Yuseong-gu, Daejeon, South Chungcheong, 34055, South Korea, University of Science and Technology, 217 Gajeong-ro, Yuseong-gu, Daejeon, South Chungcheong, 34113, South Korea; Puravankara M., Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai, Maharashtra, 400005, India; Mathew B., Department of Physics and Electronics, CHRIST (deemed to be university), Bangalore, Karnataka, 560029, India; Sharma E., Indian Institute of Astrophysics (IIA), Sarjapur Road, Koramangala, Bangalore, Karnataka, 560034, India