arXiv (All)
open access
A homogeneous analysis of archival and new low-resolution spectra of YZ Cancri
YZ Cancri is an SU UMa-type dwarf nova with sparse and heterogeneous optical spectroscopy. We present a homogeneous analysis of archival outburst-related spectra and seven new low-resolution quiescent spectra. We consistently characterize the Balmer, He I, Fe II, O I, and occasional He II and Bowen
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Challenging the archetypal intermittent radio galaxy J0111+3906. New insights from optical GTC/OSIRIS and radio VLA and LOFAR observations#1012722
- RAVE DR6 catalog of [O/Fe] ratios in dwarf and turn-off stars#934050
- HOS-NWT: an open-source numerical wave tank based on the High-Order Spectral method#153576
- Implications of Matter--Curvature Coupled Gravity on Chandrasekhar Mass Limit of White Dwarfs#684360
- Implications of Matter--Curvature Coupled Gravity on Chandrasekhar Mass Limit of White Dwarfs#682585
Record · ID 1012818
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive