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The Doppler maps constructed from hydrogen lines show a nonuniform distribution of emission in the disk similar to that observed in IP Peg. This suggests that the object can be a cataclysmic variable with tidal density waves in the disk. We have determined the component masses (M_WD =0.8 \\pm 0.22 M_sun and M_RD =0.14 \\pm 0.02 M_sun) and the binary inclination (i =78 \\pm 1.5 deg) based on"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1202.3959","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-02-17T16:46:10Z","cross_cats_sorted":[],"title_canon_sha256":"fd024d9ee7e6ff76fbc594b7bdd6e8ba404f597eb75092949e9a29ff5e85e6f1","abstract_canon_sha256":"0055539709c0cceffbe7c921e9762187e1b63928ee9af3ea63e536385a310869"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:24.049841Z","signature_b64":"EflNNe43uefRSD2OViRcMh4sRex/iuJX1pU6rhGdPqrbs9ChmHhruOs5hkzyDmyJDdTViwjOt+clZTxKHoAXAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"072ad301e5458e7a3002bffc10aad399e1d875d758583eda5d78fce12e8b96ca","last_reissued_at":"2026-05-18T01:58:24.049401Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:24.049401Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigation of the new cataclysmic variable 1RXS J180834.7+101041","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D.G. 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