◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

K. Khachatryan

4 papers hereh-index 215 citations10 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • last author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • K. Khachatryan — 2 papers, h 11
  • K. Khachatryan — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

most citedSearch for Compact Stellar Groups in the Vicinity of IRAS Sources

9 citations · 17 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2016★ 6 cited

New eruptive variable in the massive star-forming region associated with IRAS 18507+0121 source

E. H. Nikoghosyan, N. M. Azatyan, K. G. Khachatryan

Aims. We report the discovery of a strong outburst of the embedded young stellar object (YSO), namely UKIDSS-J185318.36+012454.5, located in the star-forming region associated with…

astro-ph.SR2016★ 9 cited

Search for Compact Stellar Groups in the Vicinity of IRAS Sources

N. M. Azatyan, E. H. Nikoghosyan, K. G. Khachatryan

The results of a search for compact clusters in the vicinity of 19 IRAS sources based on data from the GPS UKIDSS and Spitzer GLIMPSE surveys are presented. Overall, clusters have…

astro-ph.SR2015

The search and study of PMS stars with Ha emission

E. H. Nikoghosyan, A. V. Vardanyan, K. G. Khachatryan

One of the most prominent features of young objects in the optical range is the presence of emission lines, in particular Ha at 6563A. Therefore, Ha emission is the most common spe…

astro-ph.SR2015★ 2 cited

Statistical Analysis of stars with Ha emission in IC 348 Cluster

E. H. Nikoghosyan, A. V. Vardanyan, K. G. Khachatryan

In this work the results of the statistical analysis of the 215 stars with Ha emission in the IC 348 cluster are presented. The sample is completed to R<20.0.The optical radius is…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.